The galaxy presents an elliptical morphology, exhibiting a centrally concentrated light profile that diminishes radially outward. The core region appears to be dominated by older stellar populations, indicated by the yellowish-white hue. There is faint evidence of a blue-ish disk component surrounding the core, suggesting a relatively small amount of ongoing star formation. The overall structure appears relatively undisturbed, with no obvious signs of major mergers or tidal interactions. There might be a faint ring or other subtle feature. This object is best characterized as a relatively massive disk galaxy.
