The galaxy presents as a somewhat elliptical, diffuse object. The central region exhibits a pronounced concentration of light, appearing yellowish-orange in color, suggestive of an older stellar population. Moving outward from the core, the light gradually fades into a less defined halo. The overall structure appears relatively smooth, lacking distinct spiral arms or prominent dust lanes. There may be some subtle, faint features indicating minor disturbances in the outer regions of the galaxy, but they are not distinct. The galaxy's profile leans towards round, rather than significantly elongated. The overall color gradient implies a transition from older, redder stars in the center to a potentially younger, bluer population in the outskirts, though this is subtle. The structure does not present any signs of major merging events or significant tidal disturbances.