The galaxy presents as an elliptical-like structure with a bright, concentrated central bulge. The overall form appears relatively smooth, though some faint features are discernable in the surrounding disk. The central core exhibits a yellowish-white hue, possibly indicative of an older stellar population. Fainter, reddish patches appear slightly offset from the central bulge. These could indicate regions of ongoing or recent star formation, potentially distributed within a more extended and dusty disk. The galaxy's morphology appears slightly elongated, hinting at a mild degree of distortion. There are no obvious signs of any major tidal disturbances or ongoing merger events, though minor interactions cannot be ruled out.
