The galaxy presents as a moderately luminous, early-type system, likely an elliptical or lenticular galaxy, given its generally smooth appearance and lack of prominent spiral arm structures. The central bulge region is bright and concentrated, exhibiting a yellowish-orange hue, suggestive of an older stellar population. The outer regions show a gradual decrease in surface brightness and maintain a similar color profile to the bulge. While there is no clear indication of ongoing major mergers, there might be some evidence of minor disturbances or tidal features in the outer halo, but this is difficult to ascertain. The overall morphology is predominately smooth. The galaxy has a somewhat round shape with the possibility of a central bar or slight elongation. There appears to be modest star formation activity.
