The galaxy presents as a relatively smooth, elliptical structure with a distinct, bright central bulge. There are hints of a flattened disk component, but the morphology appears predominantly spheroidal. The central bulge exhibits a yellowish-orange hue, possibly indicative of an older stellar population, while the outer regions of the galaxy appear bluer, potentially suggesting ongoing star formation. Overall, the galaxy shows a smooth light distribution, with a higher concentration in the center. There may be some signs of minor disturbances or interactions with other galaxies, but the overall structure appears well-defined.
