This galaxy exhibits characteristics of a spiral type, though the morphology appears disturbed. It presents a moderately bright central bulge, appearing somewhat yellow in color, suggesting an older stellar population dominating this region. One of the spiral arms appears to be more prominent and extended than the other, displaying a hint of blue, suggestive of recent star formation. The galaxy's disk is not perfectly symmetrical, with some irregularities in the shape, possibly indicating ongoing interactions or mergers. There is some distortion and faint tidal features visible, which may support this hypothesis. The overall color gradient from the bulge to the outer arms suggests a varying stellar population and star formation history across the galaxy.
