The galaxy appears to be a relatively smooth, elliptical galaxy with an observed ellipticity of approximately 0.60. The central bulge region is bright and exhibits a yellowish-white color. The outer regions of the galaxy fade gradually into the background and appear somewhat bluer, potentially indicating the presence of some younger stellar populations. The galaxy exhibits no obvious spiral arm structure or dust lanes, supporting its classification as an elliptical galaxy. The overall morphology suggests a system that has largely completed its star formation, with a higher concentration of older stars in the bulge. The light distribution is centrally concentrated, and the galaxy seems to have a relatively high Sersic index. There is a possibility of a minor interaction or past merger event, given the somewhat disturbed morphology.