The galaxy appears to be a spiral galaxy, exhibiting a clear disk structure. The spiral arms are well-defined, with a relatively tight winding pattern. Two dominant spiral arms are readily apparent. A central bulge is observed; while noticeable, it does not dominate the overall structure. A subtle bar may be present, though not prominently. There is no obvious indication of a major merger event. A slight asymmetry could be an indication of tidal interactions. The galaxy's disk appears slightly inclined. The overall color suggests ongoing star formation.
