The galaxy presents as a relatively smooth, centrally concentrated object, with a luminous core that gradually fades into a more diffuse halo. The morphology appears to be largely spheroidal, with a slight deviation from perfect circularity, leaning more towards an "in between" shape. There is a noticeable lack of distinct spiral arm structure or prominent disk features. Subtle colour gradients are visible, with the core exhibiting a yellowish-orange hue, suggestive of an older stellar population, while the outer regions show a bluer tint, potentially indicating regions of recent or ongoing star formation activity, however these features are relatively weak. There is no clear evidence of major mergers or significant tidal disturbances in the immediate vicinity, though some minor asymmetry or irregularity is noted in the overall shape.
