The galaxy presents as a spiral type, though with a prominent bulge that obscures a clear view of defined spiral arms. There is a central, bright core, possibly indicative of an active galactic nucleus or a dense concentration of older stars. The disc appears somewhat disturbed, exhibiting a clumpy texture with variations in color and brightness across its extent. Patches of bluer light suggest regions of recent star formation, interspersed with areas of redder light.

The galaxy is observed at a slight angle, presenting a face-on view. No obvious signs of a major merger are visible, though the irregularities in the disk structure and the apparent disturbances may indicate a past or ongoing minor interaction. The overall morphology suggests a galaxy with a moderate stellar mass that had star formation in the past, but is currently forming new stars at a much lower rate.
