The galaxy exhibits a predominantly smooth morphology with a faint but noticeable disk-like structure. The central bulge appears bright and concentrated, displaying a yellowish hue, possibly indicating an older stellar population. The disk component is less pronounced and displays a bluer color. Overall, the galaxy appears relatively undisturbed, lacking any obvious signs of major mergers or significant tidal interactions, though there is a hint of minor asymmetry. The shape is elongated, suggesting a possible transition between elliptical and spiral morphology. The galaxy likely exhibits moderate levels of star formation.
