The galaxy presents as a moderately luminous, relatively compact system with a clear elliptical morphology. The core region appears bright and concentrated, exhibiting a yellowish hue, indicative of an older stellar population. Moving outwards from the center, a subtle transition to bluer colors can be observed in the outer regions of the galaxy, possibly indicating the presence of younger, hotter stars. While no distinct spiral arm structure is apparent, the overall shape is slightly elongated. There is no obvious indication of a major merger event or significant tidal distortions. Faint asymmetrical features might indicate a minor interaction. Overall, the galaxy appears to be a relatively evolved system, possibly a lenticular or early-type spiral, undergoing moderate star formation.
