The galaxy presents as an elongated structure, consistent with a disk galaxy observed at a high inclination. A prominent central bulge is evident, displaying a yellowish hue, indicative of an older stellar population. The disk component appears relatively smooth and featureless, suggesting either a lack of significant star formation or obscuration by dust. The overall color gradient transitions from the yellowish bulge to a slightly bluer disk, hinting at the presence of younger stars in the outer regions, although at a low rate. There is no evidence of a strong spiral arm structure or significant morphological disturbances. The galaxy appears to be relatively isolated, showing no obvious signs of recent or ongoing merger activity.
