The galaxy presents a largely smooth, elliptical morphology. There is a distinct central bulge that appears to be quite bright and concentrated, with a yellowish hue. Moving outwards from the center, the light gradually fades into a less distinct halo. There are hints of disturbed features or faint tidal tails suggesting possible minor interactions with other galaxies, or even signs of past minor mergers. There isn't a clear, well-defined disk structure visible. The overall color profile indicates a population of older stars, though there might be a low level of ongoing star formation as suggested by bluer hues mixed in with the yellowish light. The round shape is more consistent than elongated. There appears to be moderate gravitational disturbance.
