The galaxy presents a relatively compact morphology. It appears to exhibit a primarily smooth light distribution with a slight ellipticity, possibly indicative of an elliptical galaxy, though subtle features are present.

A weak disk-like structure is discernible within the primary galactic structure. It appears that there are some features such as tidal tails, however, it is difficult to say with certainty. There does not appear to be a strong central bulge, or prominent spiral arm structure.

The galaxy exhibits a somewhat mottled texture, suggesting inhomogeneity in its stellar populations. The presence of some blue-ish tinges within the disk regions may suggest the presence of younger stars, though this is a very broad estimation. The redder colors are predominant throughout, indicating an older stellar population overall. There is an overall weak color gradient from the inner to the outer regions of the galaxy.
