The galaxy presents as a slightly elliptical system with a bright, concentrated central bulge. The bulge exhibits a yellowish-white hue, suggesting a population of older stars. Surrounding the bulge is a disk component, broader in extent, with bluer tones indicative of younger, hotter stars and ongoing star formation. The disk appears relatively smooth, lacking prominent spiral arm structures, and gradually fades into the background sky. There is a slight asymmetry in the distribution of light within the disk, potentially indicating a minor interaction or disturbance. The overall appearance suggests a galaxy that is somewhere between an elliptical and a spiral type, possibly a lenticular galaxy transitioning to a more elliptical shape.
