The galaxy presents as a relatively smooth, elliptical structure with a concentrated, bright central bulge. Its overall shape appears largely undisturbed, lacking prominent tidal features or strong signs of ongoing mergers. The color profile suggests a dominant population of older stars, evidenced by the redder hues in the central region, and the overall luminosity indicates it is a massive galaxy. There is faint evidence of a subtle disk structure. There are no obvious signs of spiral arms.
