The galaxy presents as a concentrated, elliptical morphology. The central region exhibits a higher luminosity, appearing nearly spherical and slightly reddish in color. The outer regions gradually fade into the background sky, displaying a bluer hue suggestive of younger stellar populations or ongoing star formation in these areas. There is a general smoothness to the overall structure, with minimal discernible features such as spiral arms or dust lanes. Small disturbances are potentially present, but not clearly observable given the image resolution. The galaxy appears to be in a relatively quiescent state, without evidence of major merging activity.
