The galaxy appears as a centrally concentrated elliptical or lenticular galaxy with a smooth, diffuse morphology. A dominant, nearly spheroidal component is observed, exhibiting a centrally peaked light profile. The color index suggests a relatively evolved stellar population, potentially consisting of older, redder stars. There is a lack of discernible spiral arm structure or prominent dust lanes. There is a possible indication of tidal disturbance which manifests as a faint, extended halo or plume-like structure. There are no distinct signs of active star formation. The galaxy is likely at an intermediate redshift, given its observed characteristics.
