The galaxy presents as a relatively compact object with an apparent diameter of approximately 8.6 kpc. It exhibits a moderate redshift, suggesting a considerable distance from the observer.

Morphologically, the galaxy appears to be an intermediate type, possibly transitioning between elliptical and spiral characteristics. While a dominant bulge component is evident, hinting at an older stellar population, there's also a suggestion of a faint, disky structure extending outwards. Irregularities in the morphology, a very faint tidal tail, and a general fuzziness to the galactic disc suggests a past or ongoing minor merger event. The galaxy's color suggests it may be actively forming stars at a moderate rate.

Overall, the galaxy presents as a dynamically evolving system, potentially shaped by ongoing interactions and star formation processes.
