The galaxy presents a generally smooth, elliptical morphology. It exhibits a bright, concentrated central bulge, with a gradual decrease in luminosity outward. The color profile indicates a redder hue towards the center, possibly indicative of an older stellar population. Moving outward, the galaxy exhibits a slightly bluer color, potentially suggesting the presence of younger stars. The overall structure appears largely undisturbed, without any obvious signs of recent major mergers or tidal interactions. There might be a faint, diffuse disk component, however, it's difficult to distinguish from this image. The galaxy is relatively compact, showing moderate star formation activity.
