The galaxy presents a largely smooth morphology, with a dominant central bulge that appears nearly spherical in shape. The color profile suggests a relatively evolved stellar population, with a yellowish-orange hue dominating the central region, indicative of older stars. No prominent spiral arms or significant dust lanes are discernible. There appears to be very little in the way of substructure, but there is a small amount of tidal disturbance to the bottom right of the central galaxy, indicating a possible minor merger event. Overall, the galaxy seems to be largely undisturbed, with a dominant smooth component and a fairly regular shape.
