The galaxy presents as a flattened, elliptical morphology, viewed at a significant inclination to our line of sight. It exhibits a prominent central bulge, characterized by a high surface brightness and a yellowish hue, suggesting an older stellar population. A fainter, more diffuse disk surrounds the bulge, displaying a subtle color gradient from yellowish near the bulge to slightly bluer at the edges, possibly indicating the presence of younger stars and ongoing star formation in the outer regions. While distinct spiral arm structures are not readily apparent, some irregularity in the disk's surface brightness could suggest subtle, underlying spiral features. The overall light distribution appears smooth, with no obvious signs of major mergers or tidal disturbances.
