The galaxy presents as a spiral type, observed at a significant inclination to our line of sight. A prominent central bulge dominates the core region, exhibiting a yellowish hue, indicative of an older stellar population. The spiral arms are well-defined, exhibiting a relatively tight winding pattern. These arms show a bluer color, suggesting ongoing star formation. The outer regions of the disk fade gradually, indicating a decrease in stellar density with increasing radial distance. There is no apparent bar structure visible, and the galaxy does not appear to be undergoing any major interaction or disturbance based on its morphology. The general morphology suggests a relatively isolated and evolved spiral galaxy.
