The galaxy presents as a single, relatively smooth, centralized luminous object. It exhibits a generally elliptical morphology, appearing moderately rounded, though some elongation is present. The color profile suggests a population of older stars, with a dominant yellow-red hue concentrated towards the core. The outer regions appear fainter, gradually fading into the background sky, with a slightly bluer tint than the core. There is no strong evidence of prominent spiral arms or significant dust lanes from this viewing angle. There are no indications of a major merging event or significant tidal disturbances. The overall appearance is consistent with a massive galaxy, with a suppressed star formation rate.
