The galaxy presents as a spiral type, observed at a relatively face-on orientation. The central bulge appears moderately prominent and exhibits a yellowish hue, suggestive of an older stellar population. Faint spiral arms emanate from the central region, displaying a slightly asymmetric pattern. These arms seem somewhat tightly wound and are not sharply defined, with hints of flocculent structures. There are subtle color variations within the arms, which likely indicate regions of active star formation, though they are not particularly pronounced. The overall color gradient suggests a system with moderate star formation activity within the disk, with an older, more evolved stellar population dominating the central bulge. There is no clear evidence of strong tidal distortions or major merger activity, though subtle irregularities in the spiral arm structure might indicate minor disturbances. No obvious bar structure is apparent. The galaxy appears relatively isolated.
