The galaxy appears to be a relatively small, elliptical galaxy with a smooth, featureless morphology. The central bulge exhibits a higher surface brightness, gradually fading towards the outer edges. It displays a slightly elongated shape, potentially indicating a mild degree of flattening. The overall color appears to be somewhat redder, suggesting an older stellar population with a lower rate of ongoing star formation. There may be evidence of past or ongoing minor interactions or disturbances, indicated by slight asymmetries in the outer regions, though a majority of classification sources say the galaxy is not merging. Overall, the galaxy seems to be a low-mass system, and located at a moderate distance as indicated by its small size and redshift.
