The galaxy appears to be a relatively luminous, field galaxy with a redshift of approximately 0.21. Morphologically, it presents a mixed classification, showing characteristics of both smooth and disk-like structures, though a substantial portion of classifications suggest a smooth morphology. A significant portion of citizen scientists find it shows minor disturbances but is not undergoing a major merger.

The galaxy exhibits a central bulge that is elongated, surrounded by a disk. The color profile indicates the presence of both older stellar populations, evidenced by redder hues, and hints of younger, star-forming regions that might be subtly contributing to a bluer tint in certain regions. This is supported by low levels of star formation. The light appears to emanate from a region of approximately 8.6 kpc, though the overall light is not incredibly bright.

There's some visual irregularity in the galaxy's structure, potentially indicative of past interactions or internal dynamical processes. There may be a faint tidal tail.
