The galaxy appears to be a spiral galaxy with a prominent central bulge. The bulge exhibits a yellowish hue, possibly indicative of an older stellar population. Faint spiral arms are visible extending from the bulge. The arms appear somewhat flocculent and not well-defined. There is evidence of on-going or recent star formation, but the rate appears to be relatively low. There is no indication of tidal tails or significant morphological disturbances, and the light appears fairly smooth across its surface. It seems likely that this galaxy is relatively isolated.
