This galaxy exhibits a smooth, elliptical morphology. It appears elongated, almost cigar-shaped, with a noticeable central bulge that seems to dominate its overall light profile. The light from the galaxy has a warm color, suggesting an older stellar population. There is little evidence of significant dust lanes or spiral arm structures, reinforcing the impression of a relatively quiescent system. The galaxy's smooth texture indicates that it is unlikely undergoing major merging activity, and instead is in a relatively stable state. There may be minor disturbances present, but those are not immediately obvious.