The galaxy presents as a centrally concentrated object with a smooth, somewhat elliptical morphology. A significant fraction of the light is emitted from the central region, appearing yellowish-white, suggesting an older stellar population. There is evidence of bluer light extending from one side of the nucleus, possibly indicating a region of more recent star formation activity or a spiral arm structure. There is a disturbed morphology present, showing evidence of possible interaction or merger with another galaxy or tidal disturbances due to a past interaction. The overall shape is neither perfectly round nor elongated, exhibiting an intermediate axis ratio.
