The galaxy appears to be an elliptical galaxy, characterized by a smooth, centrally concentrated morphology. There is little indication of spiral arms or a prominent disk structure. The light distribution appears radially symmetric with an absence of distinct features, such as dust lanes or star-forming regions, which is consistent with an older stellar population. The galaxy exhibits a yellowish hue, suggestive of a population of evolved stars. There is no obvious evidence of ongoing major mergers or significant tidal disturbances in the galaxy.
