This galaxy presents as a relatively smooth and concentrated object. The light distribution appears centrally-concentrated with a gradual decrease in surface brightness from the core outwards. The morphology is broadly elliptical with a high degree of roundness, showing no obvious signs of strong spiral arms or a significant disk component. There's a suggestion of some minor disturbance or irregularity in the outer regions of the galactic halo, but it's not prominent, and most likely represents minor tidal interaction. The galaxy exhibits a color gradient, appearing slightly redder towards the center, suggesting an older stellar population dominates the core. The outer regions show a slightly bluer hue indicative of ongoing, but modest, star formation. Overall, this galaxy appears to be a fairly massive, moderately evolved system with a quiescent star formation rate.
