The galaxy presents a largely smooth, centrally concentrated morphology. Its light profile appears to be relatively featureless, lacking prominent spiral arms or a distinct bar structure. The galaxy exhibits a subtle ellipticity, deviating slightly from a perfect circular shape. The core of the galaxy displays a bright, concentrated luminosity, suggesting a high density of stars in the central region. A fainter, more diffuse halo extends outwards from the core, gradually fading into the background. There are possible signs of minor disturbances in the galaxy's shape, perhaps due to a small merger event. The overall color appears slightly redder, indicating a population of older stars and potentially lower star formation activity.
