The galaxy presents a generally smooth and elliptical morphology. It exhibits a bright, concentrated central bulge. The overall color appears to be yellowish-orange, suggesting an older stellar population, and possibly a lower rate of active star formation. There is a slight elongation to the galaxy's shape. No clear spiral arm structure or dust lanes are visible. The outer regions of the galaxy appear to fade gradually, indicating a diffuse stellar halo. There is no evidence of any major ongoing mergers or significant tidal disturbances in the immediate vicinity.
