This galaxy presents as a spiral type, with a clear disk component exhibiting prominent spiral arm structure. The arms appear tightly wound and extend noticeably from the central bulge. Patches of blueish coloration are observed within the spiral arms, suggestive of active star formation regions. The bulge appears moderately sized relative to the disk and is yellowish in color, potentially indicating an older stellar population. A bar structure is present that spans at least half of the length of the galaxy; the bar appears to be weak. Overall, the galaxy exhibits a relatively undisturbed morphology, showing no obvious signs of recent major mergers or tidal interactions. The galaxy displays a slightly inclined orientation relative to our line of sight.