The galaxy presents a relatively smooth, elliptical morphology. It exhibits a concentrated central bulge, characterized by a bright, diffuse glow which indicates a high density of older stellar populations. There is a subtle color gradient, shifting from a slightly bluer hue in the outer regions to a redder hue in the center. This implies that star formation is more prevalent in the outskirts, and that there is a larger population of younger, bluer stars on its rim. There is no evidence of strong spiral arms or a distinct disk component. The overall structure appears largely undisturbed, with only minor evidence of tidal features or interactions that might indicate recent merging activity. Its intermediate ellipticity suggests a shape that is somewhat in between round and elongated.
