The galaxy presents as a somewhat smooth, elongated structure. It exhibits an elliptical morphology, with a noticeable cigar shape. There is little evidence of a prominent disk or spiral arms, suggesting a later-type galaxy, possibly an elliptical. The light distribution appears relatively uniform, though there are hints of some internal variations in brightness. No significant signs of tidal disturbances or ongoing major mergers are immediately apparent, but a faint hint of a minor disturbance could exist within its halo. Its overall color appears relatively red, indicating a potentially older stellar population and reduced current star formation activity. The galaxy exhibits a moderate angular size.
