The galaxy presents a largely smooth, elliptical morphology. It exhibits a concentrated central bulge that appears to be relatively bright. The outer regions of the galaxy are more diffuse and less luminous, exhibiting a gradual decline in surface brightness with increasing radial distance from the center. The overall color is slightly redder, suggesting an older stellar population and/or significant dust obscuration within the galaxy. There are no clearly discernible spiral arms or prominent star-forming regions visible in this image. There may be a slight hint of a disk-like structure, however, it is difficult to determine. There does not appear to be any evidence of a major ongoing merger or significant tidal disturbance.
