The galaxy presents as a spiral type, exhibiting a distinct disk structure. Two well-defined spiral arms emanate from a central bulge, winding moderately outwards. These arms appear to be relatively continuous, and symmetrical. The central bulge dominates the inner region, although there is evidence of disk structure extending into this area. There appears to be no strong bar feature across the bulge. The outer regions of the disk show mottled texture indicating areas of active star formation. Overall galaxy shape appears to be unperturbed. The spiral arms display a winding consistent with intermediate coiling. Star formation appears to be occuring at a moderate to low rate, with older stars dominating the colors. The galaxy appears to be isolated, without any evidence of major interactions or mergers.
