The galaxy presents as a single, somewhat diffuse object with a centrally concentrated brightness profile. The overall color appears yellowish-white, suggestive of a stellar population dominated by older stars. The galaxy appears largely smooth in texture, lacking obvious spiral arms or significant dust lanes. The morphology is approximately round, with only a slight deviation from perfect circularity. There is no obvious evidence of tidal tails or strong gravitational disturbance, although a subtle asymmetry cannot be entirely ruled out. The galaxy likely hosts a substantial stellar mass. Ongoing star formation activity is likely present, albeit at a moderate level. There is no strong indication of recent or ongoing merger events.
