The galaxy appears to be a relatively smooth, elliptical-like structure. It exhibits a concentrated central bulge that gradually fades into the outer regions. The overall color profile seems to lean toward the redder end of the spectrum, suggesting an older stellar population. There is no apparent spiral arm structure or significant dust lane obscuration. The galaxy appears to be relatively isolated, showing no obvious signs of major interaction or merging with other galaxies, although there may be some indication of a minor disturbance in its morphology. The galaxy is moderately sized, with the light concentrated towards the center.
