The galaxy presents a generally smooth, elliptical morphology. It exhibits a concentrated, bright central bulge that fades gradually into the outer regions. The overall color profile suggests an older stellar population, potentially dominated by redder giant stars, with a hint of possible ongoing star formation. The galaxy appears to be relatively undisturbed, with no obvious signs of major mergers or significant tidal interactions affecting its structure. Its shape appears to be in between round and elliptical, with a slightly elongated form. There might be some minor distortions in the outer regions, potentially indicating a past minor interaction or accretion event.
