The galaxy presents as a fairly smooth, elliptical structure. Its light profile suggests a concentrated central region that gradually fades outwards, exhibiting a somewhat diffuse halo. The overall color is slightly red-shifted, displaying an emission spectrum weighted towards the redder bands. The isophotes appear generally round, with minimal indication of disk-like features or prominent spiral arms. There is a faint hint of disturbance, possibly related to a minor interaction, but overall the galaxy's morphology is well-defined and coherent. The brightness distribution indicates relatively quiescent star formation activity. The estimated mass range is moderate. There is no clear indication of a major merger or significant tidal disruption.
