The galaxy presents as a lenticular or possibly a tightly wound spiral structure, seen at a slight oblique angle to our line of sight. The central bulge appears prominent and relatively smooth in texture, exhibiting a yellowish-white hue, suggestive of an older stellar population. Faint, bluish extensions emanate from the central region, hinting at potential spiral arms, although they lack definitive structure and may be classified as flocculent or fragmented arms. The overall shape of the galaxy can be described as neither perfectly circular nor elongated, appearing somewhat between the two, with no apparent bar structure. There are no clear signs of on-going major mergers or strong tidal distortions, although a slight asymmetry in the outer regions could indicate minor gravitational interactions. Overall the galaxy has a faint, but detectable amount of star formation.
