The galaxy presents a smooth, somewhat elliptical morphology. There is a subtle elongation, tending towards an "in-between" roundedness. The galaxy lacks distinct spiral arm structures or a prominent central bulge. A slight colour gradient can be observed, with a slightly redder hue towards the center, possibly indicating an older stellar population, and a bluer tint towards the outer regions, which may suggest ongoing star formation. There are no signs of any major ongoing mergers. Close inspection reveals some minor disturbances or irregularities within the disk. The lack of a strong disk component and the smooth appearance suggest a classification towards early-type, possibly an elliptical or lenticular galaxy.
