This galaxy presents as a spiral type, observed at a moderate inclination. Two prominent spiral arms are visually discernible, exhibiting a loose winding pattern. The central bulge is present, appearing moderately sized within the galactic structure. A potential bar feature appears to be present, although its intensity seems mild, if it exists at all. The disk component dominates over the central bulge. There are no obvious signs of significant tidal disturbances or ongoing major merging events. The overall structure is mostly smooth with the features described.
