The object appears to be a spiral galaxy, viewed at a relatively high inclination. A prominent central bulge is observed with a bright, yellowish-white hue, suggesting an older stellar population. A faint, flattened disk extends outwards from the bulge, exhibiting a bluer color indicative of younger stars and potential star formation. The disk appears somewhat smooth, but hints of spiral structure can be discerned. There is an asymmetry in the outer regions, with a slight warp possibly present. The overall morphology suggests a galaxy that is relatively undisturbed, with minimal signs of recent major mergers or significant tidal interactions. The smoothness and color suggest it is an intermediate-mass galaxy with a mix of stellar populations.
