The galaxy presents a relatively smooth morphology, with an overall elliptical shape. The light distribution suggests a centrally concentrated structure. There are some minor disturbances to the morphology, particularly on one side of the image. This could indicate a very minor merger event, or potential tidal interactions with other objects in the vicinity. The color profile suggests an older stellar population, possibly with less ongoing star formation, due to the slightly redder appearance of the galaxy's core and central region. The galaxy does not appear to possess a significant disk component or spiral arm structure. Overall, the galaxy appears to be an early-type galaxy at a considerable distance.
