The observed galaxy presents as a spiral galaxy with a well-defined disk structure. The spiral arms appear tightly wound, originating from a central bulge region. The bulge exhibits a smooth, concentrated luminosity profile, suggesting an older stellar population. Star formation appears active within the disk, particularly along the spiral arms, indicated by the patchy distribution of bluer light. The galaxy does not appear to be undergoing a major merger, although some minor irregularities in the outer disk might suggest past gravitational interactions. The galaxy disk is oriented at a moderate inclination, allowing for a clear view of the spiral structure. A weak bar structure may be present, based on a slight elongation of the central bulge.