The galaxy presents as an elongated structure with a noticeable central bulge. Its shape deviates significantly from circular symmetry, appearing decidedly cigar-shaped. The galaxy exhibits a gradual surface brightness profile, becoming fainter toward its edges. There is evidence of a disk, and the disk may be slightly warped or irregular. The galaxy has no strong indications of active star formation, but may have intermediate levels of star formation based on the colors present. Overall, the light distribution is relatively smooth, and the light is more concentrated centrally. There is no obvious sign of any recent merger events, or tidal tail structures.