The galaxy presents as a disk-shaped system with an apparent axis ratio suggesting it is viewed at a significant inclination. The central bulge exhibits a yellowish hue, indicating an older stellar population. The disk itself appears bluer, suggestive of ongoing or recent star formation. The galaxy's light distribution, especially in the bulge, follows an exponential profile. The galaxy displays a noticeable asymmetry. This asymmetry may be indicative of past or ongoing interactions with other galaxies, although no obvious tidal features are apparent in the image.