The galaxy appears to be an elliptical galaxy, characterized by a smooth, centrally concentrated light distribution with little to no discernible spiral arm structure. The galaxy exhibits a largely spheroidal shape, appearing nearly circular in projection, with a slight suggestion of elongation. The core of the galaxy is bright and yellowish, indicating an older stellar population. The outer regions gradually fade, showing a more reddish hue, potentially signifying the presence of older, cooler stars. There is no evidence of active star formation regions. The galaxy's structure appears largely undisturbed, with no signs of ongoing or recent mergers. The outer edge of the galaxy appears sharp and distinct, not diffuse.
