The galaxy presents as a slightly inclined, edge-on spiral with a prominent, elongated central bulge. The bulge region exhibits a concentrated, yellowish-white hue, suggesting an older stellar population dominating this area. The disk component appears relatively smooth and elongated. The galaxy's apparent ellipticity indicates a significant inclination relative to the line of sight. There is no apparent distortion or tidal features indicative of major interactions, however the disk shows some slight asymmetry. The color gradient transitions gradually from the central bulge outward, suggesting ongoing star formation within the disk, possibly due to gas accretion. The overall morphology points towards a later-type spiral galaxy.
