The galaxy presents as a face-on spiral type. The structure exhibits a central bulge region with a moderate presence, surrounded by a disk structure that appears somewhat patchy, possibly indicative of on-going star formation. Faint spiral arm structures are suggested, though their definition is not strong. There is no apparent bar structure. There is little indication of a significant merger event or other major disturbances to the overall form. The galaxy appears to be a relatively isolated spiral with an estimated size that would classify it as intermediate.
