The galaxy presents a somewhat amorphous structure, though a general disk-like form can be inferred. The light distribution is not uniform; it displays a granular texture, suggesting substantial star formation regions alongside older stellar populations.

A central, slightly brighter concentration of light, possibly a bulge, is present, but not particularly dominant. The galaxy shows evidence of faint spiral arms. The disk shows minor disturbance.

Based on color indices, the galaxy contains a mix of stellar populations, with some regions appearing bluer. It is not particularly symmetric and exhibits some evidence of past or ongoing minor interactions.
