The galaxy presents as an elliptical morphology with a smooth, diffuse structure. The light profile appears centrally concentrated, with a gradual decline in brightness towards the outer regions. Color gradients are subtle, with the central region exhibiting a yellowish-orange hue, suggestive of an older stellar population. There is very little evidence of distinct spiral arms or prominent dust lanes. The galaxy appears relatively undisturbed, lacking significant signs of tidal features or ongoing mergers. It is moderately luminous, with a substantial mass. Star formation is likely low. 
