The galaxy exhibits a primarily smooth morphology, with a slight elongation along its major axis, giving it a somewhat cigar-shaped appearance. The color profile suggests a redder population indicative of older stars, with possible contribution from dust. There are no immediately apparent spiral arms or a distinct central bulge. It shows no strong signs of ongoing major mergers or significant tidal disturbances. The faintness of the surrounding halo also indicates a lack of recent, major star formation events.
