The galaxy presents as a centrally concentrated object with a smooth, diffuse appearance, suggestive of an elliptical or lenticular morphology. A slight elongation is observed, though the overall shape is relatively round. The light profile is brightest at the core, gradually fading outwards without any distinct spiral arm structures or prominent dust lanes.

A subtle color gradient is noticeable. The central region displays a slightly redder hue compared to the outer regions, which appear bluer. This color difference implies potential variations in stellar populations, with older, redder stars concentrated towards the center and younger, bluer stars populating the outskirts, or the central region may contain more dust, reddening the light.

Given the smooth morphology, the galaxy likely has low star formation rates and is a relatively massive galaxy. There is no evidence of a major ongoing merger or significant tidal disturbances in the immediate vicinity, although some minor asymmetry or faint extensions cannot be entirely ruled out with the available resolution.
