The galaxy presents a generally smooth morphology, suggesting a likely classification as an elliptical galaxy. Its shape is observed to be somewhere between round and oblong. The galaxy exhibits a central bulge that dominates the luminosity profile, with a color gradient suggesting a population of older stars concentrated toward the center. There is little evidence of spiral arms or significant dust lanes. The outer regions of the galaxy appear diffuse, lacking distinct structural features. The color profile suggests the potential for ongoing, but low, levels of star formation. There appear to be no major disturbances in the morphology indicating a major merger. There are no signs of tidal tails or other features associated with recent or ongoing interactions.
