This galaxy presents as a relatively smooth, elliptical-like structure. Its light distribution appears concentrated towards the center, indicating a prominent bulge. The overall shape is generally round, with little indication of a pronounced disk or spiral arms. The galaxy exhibits a color gradient, shifting from a bluer hue in the outer regions to a more yellow/red in the center, suggesting older stellar populations within the bulge. There is very little, if any, evidence of ongoing major mergers or tidal disturbances within the galaxy itself. There may be faint disturbances, but they are very minor. The galaxy is consistent with a high probability of being classified as smooth.
