The galaxy presents as a slightly elongated, lenticular-like structure, exhibiting a smooth, diffuse morphology. The central bulge is subtly brighter than the surrounding disk, transitioning smoothly outward. There is no apparent spiral arm structure. The overall color is consistent with an older stellar population, trending towards a redder hue. A slight asymmetry in the outer regions may indicate minor tidal interactions or past mergers, but there are no obvious signs of major disturbance. The apparent size suggests a relatively large and massive system. The galaxy appears to be relatively quiescent in terms of star formation.
