The galaxy presents as a single, centrally concentrated object with a smooth overall appearance. It appears elliptical in shape with a marked central bulge, suggesting it is a relatively evolved system. The core region exhibits a yellowish-orange hue, potentially indicating an older stellar population. Fainter, greenish emission surrounds the central region, possibly indicative of regions of ongoing, though limited, star formation. The overall smooth morphology suggests the absence of significant ongoing mergers or major disturbances. The galaxy appears relatively isolated, with no obvious close companions or tidal features readily apparent.
