The galaxy presents as a somewhat amorphous, diffuse structure with a dominant central bulge exhibiting a flattened spheroidal shape. Overall, the galaxy's light distribution appears relatively smooth. There is a slight bluing in the core suggesting some ongoing star formation. Hints of a disk-like structure are visible, potentially indicative of a spiral galaxy viewed at an angle. The edges of the galaxy are not clearly defined, fading into the background. There are signs of some disturbances in the morphology, possibly resulting from a previous minor interaction or merger.
