The galaxy presents as a spiral galaxy with a noticeable bulge. The bulge appears yellow-white, suggesting an older stellar population. The spiral arms are loosely wound and somewhat patchy in appearance. A faint blue hue is observed in some regions of the outer arms, possibly indicating areas of recent star formation. The galaxy exhibits a moderate level of disturbance, possibly due to a minor interaction or internal processes. Overall, the galaxy's color suggests a mix of stellar ages, with the bulge dominated by older stars and the spiral arms showing signs of younger stars. The galaxy is of intermediate mass.
