The galaxy presents as a relatively smooth, centrally concentrated object. Its color profile suggests an older stellar population, trending towards redder hues with a dominant yellow-orange core. The overall shape appears generally rounded, with no readily discernible spiral arms or a pronounced disk structure. There is subtle asymmetry in the outer regions, potentially indicative of minor gravitational interactions or internal disturbances. Light distribution is rather uniform with a slight elongation, not quite cigar shaped. There are hints of low-level star formation. There does not appear to be an ongoing major merger, although there might be evidence of past interactions.
