The galaxy presents a generally smooth and rounded morphology. It appears to be an elliptical galaxy, lacking prominent spiral arms or a well-defined disk structure. The galaxy exhibits a concentrated central bulge that appears bright. The color profile suggests a population of older stars, consistent with an elliptical classification. There is no indication of active galactic nuclei activity discernible within the observational limits. The galaxy doesn't seem to be undergoing major merging events or exhibiting significant tidal disturbances, further supporting its classification as an elliptical galaxy. The object is relatively compact, with an estimated size of a few kiloparsecs across.
