This galaxy presents a smooth, elliptical morphology. It exhibits a concentrated central bulge with a relatively homogenous yellowish color profile, suggestive of an older stellar population. The galaxy appears to be fairly isolated with no strong evidence of major mergers or significant tidal disturbances from nearby companions. The overall structure indicates a system transitioning toward quiescence, with low ongoing star formation activity. There is a slight elongation of the galaxy along the horizontal axis, indicating it could be elliptical.
