The object appears to be a galaxy with a moderately disturbed morphology. It is relatively compact, with an estimated effective radius suggesting a smaller size. The central region exhibits a somewhat smooth appearance, but there are indications of minor tidal disturbances, possibly due to a past or ongoing minor merger event. There is no clear spiral arm structure or bar visible. The galaxy's light distribution appears somewhat asymmetric, possibly indicating a system that has recently undergone a merger, or is still in the process of merging. The color indices from the DESI magnitudes suggest the galaxy is possibly a redder galaxy at a fairly moderate distance.
