The galaxy presents as a disk-shaped structure, observed at a high inclination. The central bulge appears moderately pronounced, displaying a smooth, concentrated light profile. The disk exhibits a discernible degree of structure, though lacking well-defined spiral arms. There is evidence of a gradual change in surface brightness from the center outwards, suggesting a relatively quiescent star formation rate. Overall color suggests a stellar population that is moderately old. There is some slight lopsidedness in its overall structure, indicating it may be slightly disturbed.
