The galaxy presents as an elliptical morphology, exhibiting a relatively smooth light distribution across its surface. The overall color appears somewhat redder, suggestive of an older stellar population and reduced ongoing star formation. There is a hint of a more concentrated central region. No strong evidence of spiral arms or significant dust lanes is readily apparent. There might be a faint hint of tidal interactions or disturbances in the immediate vicinity, although it is not definitively clear from the image. The galaxy appears relatively isolated, with no obvious nearby companions undergoing a major merger. The overall structure suggests a system that has likely undergone significant dynamical relaxation.
