The observed galaxy appears to be a spiral galaxy, with a discernible disk structure. Spiral arms emanate from a central, brighter bulge region. These arms are tightly wound, displaying a noticeable blueness indicative of ongoing star formation. The bulge appears relatively small, and the disk itself is moderately inclined to our line of sight. Evidence suggests the presence of a bar feature within the central region, although it is difficult to assess the bar's strength. The spiral arms exhibit a flocculent structure, displaying several distinct clumps and regions of enhanced star formation activity. The overall shape of the galaxy deviates somewhat from a perfect circle, exhibiting a slight ellipticity. The galaxy does not appear to be undergoing any major mergers, only minor disturbance.
