The galaxy presents a generally smooth, elliptical morphology, although it is neither perfectly round nor elongated. There is some deviation from a purely smooth appearance. The galaxy exhibits a concentrated central bulge that dominates its luminosity profile. The bulge appears to have a yellowish hue, indicative of an older stellar population. Surrounding the bulge is a more diffuse halo or disk component that appears bluer, suggesting the presence of younger stars and/or ongoing star formation, albeit at a low rate. The galaxy does not appear to be undergoing any major mergers or significant tidal disturbances. Evidence of minor interactions is faint if present. The overall structure suggests a relatively evolved system transitioning towards a more passive state.
