The galaxy appears to be a relatively smooth, centrally concentrated system. It exhibits a roughly elliptical morphology, with an apparent lack of strong spiral arm features. There is a discernible color gradient, transitioning from a yellowish-white core region to a bluer hue in the outer regions. The central bulge is prominent, suggesting a substantial population of older stars. The galaxy is not perfectly symmetrical, hinting at possible past or ongoing minor gravitational interactions with another galaxy, or perhaps an internal disturbance. The outer regions display some faint, diffuse structure, potentially indicating a disk component or tidal debris. There is no readily apparent indication of a major merger or significant starburst activity from this image alone.
