The galaxy presents as a moderately luminous, elongated system, suggestive of an elliptical morphology, although a highly inclined disk galaxy cannot be ruled out. The light distribution exhibits a centrally concentrated bulge with a gradual decrease in surface brightness towards the outer regions. The core of the galaxy appears to be a yellowish-white hue, possibly indicating an older stellar population. There are hints of bluer colors in the outer regions, which might indicate more recent star formation activity, though this is less evident. The galaxy appears relatively undisturbed, with no obvious signs of major mergers or tidal interactions. The overall structure seems relatively smooth and lacks prominent dust lanes or spiral arm features. The apparent lack of significant star formation suggests that the galaxy is relatively quiescent.
