The galaxy presents a relatively smooth, elliptical morphology. It appears moderately rounded, with no obvious signs of a distinct disk structure. The central bulge exhibits a slightly brighter concentration of light, fading outwards into a more diffuse halo. There is no apparent spiral arm structure or bar.

The color profile of the galaxy suggests a population of older stars, indicated by its yellowish-orange hue. There's no evidence of significant dust lanes or prominent star-forming regions, which supports its classification as a relatively quiescent galaxy. Minor disturbances may be present, but the overall form appears mostly relaxed, with no significant signs of ongoing merging or major interactions with other galaxies.
