The galaxy appears to be a relatively smooth, disk-like galaxy with a possibly disturbed morphology. It is a faint and relatively small, with an approximate physical radius of 15 kpc. It exhibits a slight elongation, deviating from a perfectly circular shape. The galaxy's light is concentrated towards the center, with a gradual decrease in brightness towards the outer edges. It appears yellow indicating it could be composed of an older stellar population with lower ongoing star formation. There is no evidence of a spiral arm structure or a prominent central bulge. Given the observed morphology, there is possibility of an ongoing minor interaction, or recent merger.
