The galaxy presents an elongated, cigar-shaped morphology. It appears predominantly smooth in structure, lacking prominent spiral arms or a distinct bulge. The galaxy exhibits a generally elliptical profile with a slight extension along its major axis.  Color gradients suggest a possible redder core region, transitioning to slightly bluer hues in the outer regions, potentially indicating varying stellar populations. The galaxy appears relatively isolated, with no immediately apparent signs of tidal interactions or mergers, although a subtle minor disturbance within the structure can not be ruled out.  The light distribution is relatively smooth.
