The galaxy presents as a moderately bright, compact object with a relatively smooth appearance. There is some indication of a slight disk-like structure, but the overall impression is that of a spheroid. The galaxy appears to exhibit a subtle color gradient, with a slightly bluer hue in the central regions transitioning to redder tones towards the outer edges. This suggests a radial variation in stellar populations and/or dust content, possibly indicative of ongoing or recent star formation in the core. There is no obvious evidence of a major ongoing merger or significant tidal disturbances, though minor interactions cannot be ruled out at this resolution. The overall shape appears somewhat elliptical, trending towards a more rounded morphology.
