The galaxy appears to be a spiral type, exhibiting a distinct disk structure. The spiral arms are tightly wound around a central bulge. The disk presents a mottled texture, suggesting areas of active star formation. Overall the galaxy appears relatively isolated, exhibiting a general symmetry. The colour distribution indicates a higher concentration of older stars in the central bulge. There are no apparent signs of a strong bar structure. Faint outer regions are visible around the disk. The system presents a face on view relative to our line of sight.
