The galaxy presents as a relatively smooth, elliptical-like structure, with a concentrated central bulge. The light distribution appears centrally concentrated, with a gradual decrease in intensity towards the outer edges. The galaxy exhibits a dominant yellowish-white hue in its core, suggesting a population of older stars, while the outer regions show hints of bluer tones indicating some younger stellar populations, though faint. There is no clearly defined spiral arm structure or bar visible. Faint, diffuse features extending beyond the main body of the galaxy might indicate tidal interactions or faint stellar halos. Overall, the galaxy appears relatively undisturbed, with no major signs of ongoing mergers or strong tidal distortions. The shape is more in between round and elongated. It seems to be a large galaxy with an estimate of its star formation rate suggesting it's not highly active. 
