The galaxy appears to be an elliptical galaxy, displaying a generally smooth, rounded morphology. Its core presents a concentrated region of high luminosity, exhibiting a reddish-yellow hue that transitions to a dimmer, slightly bluer halo. There's little discernible disk structure; rather, light distribution falls off relatively smoothly from the center. There's no clear evidence of spiral arms, bars, or ongoing major merging events in the visible light. The redder core suggests an older stellar population, while the slightly bluer outer regions indicate at least some degree of recent star formation. No significant tidal tails or distortions are visible, suggesting this galaxy is relatively relaxed and has not undergone recent major interactions.
