The galaxy presents a distinct spiral structure. Two prominent spiral arms emanate from the central region, displaying a relatively loose winding pattern. A bar-like feature appears to be present within the central bulge, but it may be faint or weakly defined. The bulge appears to be of a small to moderate size relative to the overall disk of the galaxy. The color distribution indicates active star formation regions within the spiral arms, evidenced by bluer hues, while the central bulge exhibits a yellower, potentially indicative of an older stellar population. The galaxy exhibits no obvious signs of major merging activity but may be undergoing a minor disturbance, as there are some asymmetries in the distribution of light. Overall, the galaxy appears to be a relatively well-formed spiral galaxy, potentially in a stage of significant star formation.
