The galaxy presents as a centrally concentrated object, exhibiting a relatively smooth, elliptical morphology. The light profile appears to gradually decrease from the core outwards, with no distinct spiral arm features or prominent dust lanes visible in the image. There is a slight elongation, giving it an in-between, not-quite-round shape. Based on the color index derived from the DESI magnitudes, it is appears to be redder in color, indicating an older stellar population with a suppressed star formation rate. The galaxy does not show any signs of major merging activity or significant tidal disturbances.
