The galaxy presents as a generally smooth and rounded object. It exhibits a concentrated central bulge that transitions smoothly into an extended halo. There's a subtle color gradient visible, with a slightly yellower hue towards the core, suggesting an older stellar population concentrated centrally. The outer regions of the galaxy appear bluer, which implies the presence of younger, hotter stars potentially forming in the disk or halo. There are no readily apparent spiral arms or significant dust lanes, but there are some faint distortions. Based on the lack of substantial disk features, it's likely an elliptical galaxy.
