The galaxy presents as a single, somewhat smooth, elliptical-like structure. It exhibits a concentrated central bulge, where the intensity of light is the highest. The color gradient suggests an older stellar population, appearing more yellow/red in the optical bands, especially towards the center, indicating relatively low levels of current star formation. The outer regions of the galaxy appear fainter and more diffuse, with a gradual decrease in surface brightness, possibly indicative of an extended halo. There is no apparent spiral arm structure or other significant morphological features such as strong tidal tails or evidence of recent major mergers. The overall shape appears nearly round but has a slight elongation towards the horizontal axis. There might be some minor disturbances on the outskirts, but these are difficult to distinguish due to the resolution of the image.
