The galaxy presents a spiral morphology, with two clearly defined spiral arms extending from a central bulge. The arms exhibit a medium winding, appearing neither tightly wound nor loosely dispersed. The bulge appears to be of moderate size relative to the disk, showing a distinct yellowish hue suggesting an older stellar population. Patches of blue are observed within the spiral arms, indicative of ongoing star formation regions. The galaxy does not appear to be significantly disturbed, lacking obvious signs of recent major mergers. A weak bar structure may be present. Overall, the galaxy seems to be a relatively normal spiral galaxy undergoing active star formation within its spiral arms.
