The galaxy presents as a single, relatively smooth and concentrated object. It appears elliptical or lenticular, displaying a centrally concentrated bulge. There is no obvious spiral arm structure or prominent dust lanes. The galaxy exhibits a moderate ellipticity, appearing somewhat elongated, but not cigar-shaped. There are no strong indications of a major ongoing merger, although subtle irregularities could suggest minor gravitational interactions or disturbances. The color profile is relatively uniform, with a tendency toward redder hues, indicative of an older stellar population and limited ongoing star formation activity.
