The galaxy presents as a relatively smooth and rounded structure. It exhibits a centrally concentrated luminosity profile, with the brightest region appearing towards the center. There are hints of a faint, extended halo surrounding the brighter central region, suggesting a gradual decrease in stellar density with increasing radial distance. No distinct spiral arms or bar features are readily apparent in the image. The overall color of the galaxy appears to be yellowish-orange, suggestive of an older stellar population. The absence of prominent blue regions indicates a relatively low rate of recent or ongoing star formation. There are no obvious signs of major tidal disturbances or mergers.