The galaxy appears to be a relatively smooth, elliptical system. It exhibits a high degree of central concentration with a gradual decrease in luminosity outwards from the core. The overall shape is nearly circular. No distinct spiral arms, bars, or significant dust lanes are readily apparent. The galaxy's color suggests a population of older stars, with a yellowish-red hue dominating the light emitted. There is no obvious evidence of ongoing major mergers or tidal disturbances, the galaxy's structure appears largely undisturbed. A minor asymmetry might exist, but it's difficult to confirm without higher resolution imaging. It presents a generally relaxed morphology.
