The galaxy appears to be a spiral type, exhibiting a distinct disk structure. The disk is oriented at a moderate inclination relative to our line of sight. Two prominent spiral arms are discernible, displaying a medium winding pattern. The central bulge is moderately sized and features a bright core, suggesting a considerable stellar population and possibly an active galactic nucleus. There is some evidence of a bar structure extending from the central region. The arm color appears to be bluer than the bulge, suggestive of active star formation within the spiral arms. The disk shows irregularities, potentially indicating minor gravitational interactions or ongoing accretion events. The overall color suggests a population of both young and old stars.
