The galaxy presents as a relatively smooth, elliptical form. Its light is concentrated toward the center, suggesting a prominent bulge. The color profile indicates an older stellar population, with a yellowish-red hue dominating the central region. Fainter, bluer light is visible towards the edges of the galaxy, hinting at some ongoing, albeit subdued, star formation activity. The galaxy appears undisturbed, lacking any obvious tidal features or signs of recent mergers. There are slight indications of asymmetry, possibly caused by a minor interaction in the past. The overall morphology is consistent with a quiescent galaxy that is relatively evolved.
