The galaxy presents as an elliptical or lenticular type. It exhibits a smooth, centrally concentrated light distribution, with minimal discernible spiral arm structure. The central bulge is prominent and appears almost spherical, with a yellowish color indicative of an older stellar population. The outer regions show a gradual decrease in surface brightness and a slightly more reddish hue, potentially due to the presence of dust or a population of older, redder stars. There is no strong evidence of ongoing major merger activity, although some subtle irregularities in the outer regions might suggest a past minor interaction. The galaxy appears relatively isolated within the observed field.
