The galaxy presents as a relatively smooth, disk-shaped structure. It appears elongated, displaying a cigar-like shape. A bright, concentrated central bulge is evident, with a yellowish-orange hue. The disk itself is less defined, showing hints of structure but lacking prominent spiral arms. The color of the disk transitions to a bluer shade, indicating the presence of younger stars. There are no signs of major mergers or significant tidal disturbances in its immediate vicinity. Overall, the galaxy's appearance suggests it may be a late-type spiral or lenticular galaxy undergoing relatively low levels of star formation.
