The galaxy presents as a relatively smooth, elliptical-like structure with a concentrated central bulge that emits a strong yellowish light. The core appears to be fairly dense, exhibiting a high degree of luminosity. There's a gradual decrease in luminosity extending outwards from the central bulge into the outer regions of the galaxy, which show less distinct features. There appears to be minimal disk structure; the galaxy has a generally amorphous profile. Any spiral arm structures are not well-defined. There is no indication of strong active star formation, based on the lack of intense blue emission. Signs of recent merger activity or significant tidal disturbances are also absent. The shape appears mostly rounded, with only a slight ellipticity. Overall, the galaxy seems to be a relatively evolved system, with an older stellar population dominating its observed light.
