The galaxy presents as a moderately sized object, exhibiting a disk-like morphology. The central region appears significantly brighter, potentially indicating a central bulge. There is a suggestion of spiral arm structure, although it is somewhat indistinct and possibly disrupted. Patches of bluer light are visible within the disk, possibly indicating regions of active star formation. Overall, the galaxy exhibits some degree of disturbance in its structure, suggestive of past or ongoing interactions.
