The galaxy presents as a single object with a generally smooth appearance, though it displays possible features indicative of a past or ongoing interaction. The galaxy’s morphology appears elongated, almost cigar-shaped, suggesting it could be an elliptical galaxy or a spiral galaxy viewed at an angle.

There's a noticeable color gradient within the galaxy. A central, bright region exhibits a bluer hue, indicative of a stellar population with recent or ongoing star formation activity. This region is less concentrated than the yellowish region. Extending away from the blue region, there is a more diffuse, yellowish component. This may represent an older stellar population, or regions of dust obscuring the bluer light from behind. The presence of both blue and yellow light suggests the presence of both young and old stars. 

There's an indication of disruption or merging, seen as a possible tidal tail or a slightly disturbed morphology on one side of the galaxy. This faint extension could be indicative of gravitational interaction with another galaxy. The disturbance implies some ongoing merging.

The overall magnitude suggests this is a reasonably luminous galaxy for its distance.
