The galaxy presents a generally elliptical morphology. It exhibits a bright, concentrated central bulge that appears yellowish-white, suggesting an older stellar population. Extending outward from the central bulge is a fainter disk component, which has a bluish tint indicating regions of ongoing star formation. The galaxy is not perfectly circular; it shows a slight elongation along one axis, giving it a somewhat cigar-shaped appearance. There is no apparent dust lane or obvious spiral arm structure visible in this image. The overall structure indicates a galaxy that is relatively smooth. There is no strong evidence of a recent or ongoing major merger event, although minor asymmetries in the outer regions cannot be entirely ruled out. The light distribution suggests a system with a dominant bulge and a less prominent disk.
