The galaxy presents a generally smooth morphology. It appears somewhat elliptical in shape, leaning towards an elongated form but not excessively so. The light distribution is concentrated towards the center, suggesting a relatively dense nucleus. While smooth in appearance, there's a subtle hint of a possible disk or arm-like feature on one side, though this is not definitively resolved. The color profile indicates a mix of stellar populations, with the core appearing more yellowish, suggesting older stars, and the outer regions showing hints of bluer light, potentially indicating younger star formation regions. There is no strong evidence of ongoing major mergers or tidal disturbances, though the aforementioned subtle structural feature could imply minor interactions or internal processes. Overall, it seems to be a moderately massive galaxy that has largely settled into a quiescent phase, but still retains some localized star formation.
