The galaxy presents as a relatively compact object with an apparent size indicating a non-negligible physical extent. Its light profile is predominantly smooth, suggesting a morphology tending towards an elliptical or lenticular classification. While a disk structure is not immediately evident, a slight flattening or asymmetry cannot be entirely ruled out. 

The color indices derived from DESI magnitudes suggest a redder overall stellar population. This could be indicative of an older stellar population, lower levels of on-going star formation, or significant dust obscuration. Star formation may occur but at low rates. It appears that a significant number of mergers may be occurring.
