The galaxy presents a generally smooth, elliptical morphology. It exhibits a bright, concentrated central bulge that gradually fades outwards into a less luminous, extended halo. The overall color profile suggests a population of older stars, indicated by the yellowish-orange hue of the bulge. There is some evidence of bluer light in the outer regions, possibly indicative of more recent, although likely modest, star formation activity. There are no obvious signs of spiral arm structure or a prominent disk component. The galaxy appears relatively isolated, with no immediate tidal distortions or nearby companions visibly interacting with its structure. There is a slight asymmetry to the outer isophotes.