The galaxy presents a relatively compact morphology, with an apparent size indicative of a moderately distant object. The light profile appears centrally concentrated, with a smooth, diffuse halo surrounding a brighter core. The color gradient transitions from a bluish central region, potentially indicating younger stellar populations or active galactic nucleus activity, to a more yellowish/reddish outer region, suggesting older, redder stars. There appears to be some minor disturbance of the morphology within the central core. This could be due to tidal interactions or ongoing merging activity, although no strong tidal tails or extended structures are immediately apparent. There is a faint disk feature around the center that is heavily disturbed. No resolved spiral arms or prominent dust lanes are readily discernible in this image.
