The galaxy presents as a spiral type, observed at a slight angle relative to face-on. Two prominent spiral arms emanate from a central, moderately sized bulge. These arms are relatively well-defined and appear to be moderately wound. There is evidence of ongoing star formation within the arms, indicated by the clumpy, patchy distribution of light and subtle color variations, likely representing HII regions. The central bulge appears relatively smooth and uniform in color, suggesting an older stellar population. The galaxy appears to be relatively isolated, showing no immediate signs of a major merger or significant tidal disruption. However, there is a subtle asymmetry in the overall structure of the galaxy, which could indicate a minor interaction or disturbance. A faint bar may be present spanning across the bulge of the galaxy.
