The galaxy presents a flattened disk-like morphology, indicating a spiral or lenticular structure. Two distinct spiral arms are visible. The arms display a moderate winding, neither tightly coiled nor loosely extended. The central bulge appears relatively small compared to the overall disk size and possesses a yellowish hue, possibly indicating an older stellar population. Bluer regions are distributed throughout the spiral arms, suggesting active star formation. There is no indication of a strong bar feature bisecting the bulge. The galaxy exhibits a slight degree of asymmetry in its morphology and color distribution, which could indicate a minor gravitational interaction with a satellite galaxy.
