The galaxy presents a generally smooth morphology, exhibiting a somewhat elliptical shape. The central region displays a concentrated luminosity with a distinct reddish-orange hue, potentially indicative of an older stellar population and/or dust obscuration. Moving outwards from the center, the color profile transitions towards a bluer tone, suggesting the presence of younger stars. The overall structure appears largely undisturbed, without readily apparent signs of major mergers or strong tidal interactions. There might be minor disturbances, though they are subtle. The galaxy is likely undergoing star formation, although at a relatively low rate.
