The galaxy appears to be a spiral type, although exhibiting some degree of disturbance. There is a slight, but discernible, disk structure, with hints of spiral arms. These arms appear somewhat flocculent and asymmetric, which suggests possible interactions or internal disturbances. There is no obvious central bulge, suggesting a smaller bulge or a later-type spiral classification. The color profile shows a moderate presence of bluer light, indicating ongoing star formation. Overall, the galaxy exhibits characteristics consistent with possible minor merger activity.
