The galaxy presents as a smooth, centrally concentrated object. Its overall shape is elliptical, tending toward moderately rounded, with no obvious presence of spiral arms or a distinct disk structure. The light profile appears to be dominated by an older stellar population, as suggested by the yellowish-red hue of the central region, which likely indicates a population of evolved stars. There is some evidence of a faint, slightly bluer halo surrounding the core, possibly indicating a small amount of ongoing star formation. No signs of major mergers or tidal disturbances are immediately apparent.
