The galaxy presents as a tilted disk with an elliptical morphology. It exhibits a prominent bulge that appears quite smooth and concentrated, with a yellowish hue suggesting an older stellar population. The disk component shows subtle spiral arm features, though they are not sharply defined. Blueish tints are present in the outer regions, indicative of younger, hotter stars, and perhaps ongoing star formation. There appears to be some dust obscuration, mainly near the equatorial region of the disk, slightly distorting the light from the bulge. The galaxy is elongated, and the narrowness suggests we are viewing it at a high inclination angle, close to edge-on. There is no immediately apparent evidence of recent major merger activity.