The galaxy presents as a spiral galaxy with a redshift of approximately 0.10. The galaxy's apparent size is relatively compact, suggesting a small physical size and distance.

Visually, it displays a prominent central bulge, which appears relatively smooth and concentrated. The disk component is noticeable, with hints of spiral arm structure. The arms are somewhat flocculent in appearance.

There is some evidence of tidal disturbances, possibly indicating an ongoing interaction with another galaxy, although it might be an artifact.

The light distribution suggests a mix of stellar populations, with older, redder stars dominating the bulge, and regions of bluer, younger stars present in the disk, possibly in areas of active star formation.
