The galaxy presents as a resolved object exhibiting a predominantly elliptical morphology. The central region displays a high surface brightness and a yellowish-white hue, suggesting an older stellar population. There is a slight flattening observable, deviating from a perfectly circular shape. The outer regions fade gradually into the background, showing a smoother distribution of light with hints of a disk shape. The colour profile indicates a redder population in the central bulge, transitioning to slightly bluer colours in the outer regions, suggestive of some ongoing star formation. There is little evidence of strong spiral arm structure or significant dust lanes. The overall structure appears relatively undisturbed, without any apparent tidal features or signs of a major merger event.
