The galaxy appears as a relatively compact object with a bright central core, likely indicating a significant concentration of stars. Its morphology is suggestive of a disk-like structure, though it is not clearly defined. The light distribution appears somewhat asymmetric, with a slightly elongated form along one axis, possibly indicating the presence of faint spiral arms or a tidal disturbance. The central region exhibits a bluish hue, potentially signifying active star formation, while the outer regions show a shift toward redder colors. The lack of strong, distinct features hints at a relatively smooth stellar distribution within the galaxy. Close inspection of the galaxy reveals some distortion from what would be expected of an elliptical or spiral shape, and has what appears to be a companion galaxy to its left.
