The galaxy appears roughly elliptical in shape with a concentrated, bright central bulge. There is some evidence of structure and faint arms, though these are not well-defined. The color profile suggests a mix of stellar populations, with a bluish tint in the central region indicating the presence of younger, hotter stars. The outer regions exhibit a redder hue, potentially indicating older stellar populations or dust obscuration. The overall texture is relatively smooth, with some areas appearing less uniform, possibly due to minor disturbances or ongoing interactions. The surrounding halo is faint, and not clearly defined, but some evidence of tidal disruption in areas suggesting merger activity.
