The galaxy presents as a centrally concentrated elliptical or lenticular system. It exhibits a smooth, diffuse morphology with a notable lack of distinct spiral arm structures. The light profile appears concentrated towards the core, suggestive of an older stellar population. The color indices indicate a redder overall color, potentially indicative of a low star formation rate and a dominant population of older, redder stars. There is no obvious evidence of ongoing major mergers or tidal disturbances. The shape is predominately in between round and cigar shaped.
