The galaxy presents as a relatively smooth, elliptical morphology. It exhibits a concentrated central bulge, surrounded by a more diffuse halo. The color profile suggests an older stellar population, exhibiting a reddish-yellow hue in the core, likely due to evolved giant stars. There is little evidence of spiral arm structure or prominent dust lanes. The galaxy's overall roundness indicates a possible classification as an E4 or E5 elliptical galaxy. There's no obvious sign of major mergers or tidal disruptions. Faint color variations within the halo may suggest variations in the stellar population or metallicity, however, they could also result from image noise. Overall, the galaxy appears relatively undisturbed and evolved.
