The galaxy presents as a generally smooth, elliptical object. Its core region appears bright and concentrated with a yellow-red hue, suggesting an older stellar population. The galaxy exhibits a gradual decline in luminosity moving outwards from the center towards its periphery. While the core region is defined, its outer edges appear diffuse, without distinct spiral arm structures or prominent dust lanes visible in this image. There are hints of a flattened disc-like structure, but this is not well-defined, lending to its classification as likely an elliptical galaxy. There are no apparent signs of any major ongoing merger events, although there are hints of possible minor tidal disturbances in the outer regions. 
