This galaxy exhibits a generally smooth morphology with a relatively high degree of central concentration. It presents an elliptical, albeit slightly elongated, shape. The primary color appears to be a yellowish-white, indicative of a stellar population dominated by older stars. The galaxy lacks any readily apparent spiral arm structure or significant dust lanes. A slight color gradient may be present, suggesting some degree of ongoing, or recent, star formation, but at a low rate. There is no clear indication of any major merger event in the galaxy's recent history, though subtle disturbances cannot be entirely ruled out. Overall, the galaxy seems to be a relatively undisturbed, evolved system.
