The galaxy presents a generally smooth, elliptical morphology. Its color profile suggests the presence of an older stellar population, with a concentration of redder hues towards the central region. The overall structure appears largely undisturbed, lacking any obvious signs of ongoing mergers or major tidal interactions. The galaxy shows a slight elongation, but overall, it is closer to being round than cigar-shaped. There is evidence of some ongoing star formation, with a small amount of green color apparent, however this appears limited and does not dramatically affect the elliptical morphology.
