The galaxy presents an overall elliptical morphology, displaying a smooth, concentrated light profile with a bright central bulge dominating the luminosity. The galaxy exhibits a slight flattening, deviating minimally from a perfectly circular shape. The color profile shows a strong red component, particularly concentrated in the core, suggesting an older stellar population. Fainter, bluer hues are observed in the outer regions, potentially indicating younger stars or ongoing, albeit subdued, star formation. There is no prominent spiral arm structure or dust lane visible. Faint, diffuse extensions extend from the main body of the galaxy, hinting at a possible halo or tidal features, though no significant signs of a major ongoing merger or strong tidal disruption are apparent.
