The galaxy presents as a somewhat amorphous structure with a generally elliptical shape. There's an apparent concentration of light towards the center, suggesting a possible bulge component. The light is not uniformly distributed; there are areas that appear brighter and more diffuse, as well as regions where the light appears to fade gradually. There are hints of spiral structure, though these features are not sharply defined and could be indications of tidal disturbances. The galaxy exhibits a range of colors, with some areas appearing bluer, possibly indicating regions of recent or ongoing star formation, and other regions appearing redder, perhaps indicating older stellar populations. The galaxy shows evidence of a possible interaction or past merger event, which is causing some irregularity in its overall morphology.
