The galaxy presents a relatively smooth, elliptical morphology. It exhibits a noticeable central bulge that appears bright and concentrated. Moving outward from the center, the galaxy appears more diffuse. The observed color gradients suggest some degree of stellar population variation; the central bulge may be dominated by older, redder stars, while the outer regions show bluer colors, possibly indicating younger stellar populations or ongoing star formation. The disk is relatively flat, and is approximately 4 kpc in radius. Overall, the galaxy appears to be a relatively massive system with a low star formation rate. The galaxy does not appear to be undergoing any major merger activity, but there may be some minor asymmetry or disturbance in its structure. The overall shape is in between round and cigar shaped.
