The galaxy presents as a somewhat asymmetrical, disk-like structure. It is not perfectly circular. There is evidence of a possible central bulge, appearing as a concentration of light. Multiple regions of star formation are indicated by the presence of bluer light as well as orange colored areas. Faint spiral arms, or at least disrupted arms, are weakly suggested by the light distribution. It is in an active period of star formation. There is some indication of tidal interactions and faint, disturbed features, suggesting a possible interaction or merger event, though no major disturbances are visible. Overall, it looks to be a moderate-sized galaxy.
