The galaxy exhibits a flattened, elliptical morphology, suggesting it is likely an early-type spiral or lenticular galaxy viewed at a shallow angle. A prominent bulge dominates the central region, appearing smooth and concentrated, and displaying a yellowish-orange hue indicative of an older stellar population. Fainter, bluer light suggests the possibility of ongoing star formation, albeit at a lower rate. The overall structure appears relatively undisturbed, with no strong evidence of major mergers or tidal interactions. There might be a very slight warping to one side of the disk, though the resolution is a bit too low to make a definite statement. 
