The galaxy presents a generally elliptical morphology. Its core is luminous and concentrated, displaying a yellowish-gold hue, indicative of an older stellar population. This core region appears relatively smooth and lacks distinct features. Extending outwards, the galaxy exhibits a fainter, diffuse halo. The galaxy appears relatively undisturbed, showing no signs of major merger events or significant tidal interactions with neighboring galaxies. The apparent color gradient suggests a potential radial variation in stellar population, with the core being dominated by older, redder stars and the outer regions potentially containing a younger, bluer population, albeit subtly. The galaxy's elongated shape deviates slightly from a perfect sphere, leaning towards a more flattened, ellipsoidal form. There is little evidence of significant dust lanes or prominent spiral arm structures within the visible light spectrum.
