The galaxy presents an elliptical morphology, exhibiting a relatively smooth, centrally concentrated light distribution. A distinct, bright core is visible. The galaxy's color profile suggests a primarily older stellar population, with a redder hue dominating the central bulge. Fainter, bluer regions may be present in the outer disk, implying some ongoing, albeit low-level, star formation activity. There are some subtle disturbances in the outer regions of the galaxy, hinting at a possible past or ongoing minor interaction or merger. These disturbances might be tidal features, but could also simply be internal structures. The overall appearance is that of a galaxy that has largely settled into a relatively quiescent state, with potential for future interactions.
