The object in question appears to be an elliptical galaxy, exhibiting a generally smooth and rounded morphology. A distinct central bulge is visible, appearing bright and somewhat yellow-red in color, potentially indicating a population of older stars. The galaxy lacks any readily apparent spiral arm structure or significant dust lanes, further supporting its classification as elliptical. There may be a faint, diffuse halo surrounding the central region, suggesting an extended distribution of stars. There is no obvious indication of tidal disruption or ongoing merger activity.
