The galaxy presents as a somewhat elongated, cigar-shaped structure. Its morphology appears relatively smooth, with a diffuse light distribution suggesting an elliptical or lenticular classification. The primary body of the galaxy exhibits a color gradient, appearing bluer in the central regions and shifting towards redder hues in the outer edges. This could indicate ongoing star formation in the core and an older stellar population towards the outskirts. There is a slight suggestion of possible tidal features or minor disturbances, such as faint plumes or asymmetries, implying a possible past or ongoing interaction with another galaxy, although it is difficult to verify from this image. The galaxy has a notable red shift, which, combined with its luminosity suggests it is a reasonably massive and actively star-forming galaxy.
