The galaxy presents as a centrally concentrated object, exhibiting a smooth and largely featureless morphology. The light profile appears centrally peaked with a gradual decrease in surface brightness outwards. There appears to be a bright, approximately round central region with an extended, slightly elliptical halo. The overall color profile suggests a redder core transitioning to a bluer halo, indicative of potentially older stellar populations in the center. There is no obvious spiral arm structure or significant dust lane obscuration visible at this resolution. Signs of recent or ongoing major mergers, such as tidal tails or distorted morphology, are absent. There may be a small hint of minor disturbances in the outer halo, but it could also be noise. It is likely that this galaxy is an elliptical galaxy.
