The galaxy presents as a relatively smooth, elliptical object. It exhibits a concentrated central bulge region, displaying a somewhat redder hue in comparison to the outer regions. The observed color gradient implies a potential variation in stellar populations, with the core possibly dominated by older, redder stars. The outer regions of the galaxy appear less defined, with a more diffuse and slightly bluer cast, indicative of the presence of younger stars or ongoing star formation, albeit at a modest rate. There's a suggestion of a flattened or elongated shape, although the overall structure lacks distinct spiral arms or prominent features. No strong signs of significant tidal disruption or major merger activity are readily apparent, though a minor disturbance cannot be entirely ruled out at this resolution. The galaxy appears to be a reasonably massive system.
