The galaxy presents a somewhat elliptical morphology, appearing more rounded than cigar-shaped. A central bulge is discernible, exhibiting a yellowish hue, indicative of an older stellar population. Fainter, bluer regions extend outward from the central bulge, hinting at regions of more recent star formation within a disk-like structure. The galaxy appears relatively smooth, although there is subtle evidence of a possible minor disturbance or interaction. The galaxy's overall color profile suggests it is an intermediate type, residing between a spiral and an elliptical classification. A merging event appears to be present in the object.
