The galaxy presents as a concentrated, somewhat elliptical form with a bright, yellowish core. The central region displays a smooth, blended light profile suggesting an older stellar population. The outer regions appear fainter with a slightly irregular shape, possibly indicating minor disturbances or ongoing interactions. There are hints of redder regions indicating potential areas of on-going star formation. Overall, the galaxy seems to be a relatively massive object, with evidence of a developed structure and a significant central bulge. There is a slight asymmetry to the light distribution in the halo that warrants further investigation.
