The galaxy presents as an elongated, cigar-shaped structure. It appears to be a disk galaxy seen at a high inclination. The central region shows a concentration of light, likely corresponding to the galactic bulge. The bulge appears relatively smooth, with a yellow-white color, suggesting a population of older stars. Fainter, bluer light extends from the central region, indicating the presence of a disk. There is a lack of clearly defined spiral arm structure, potentially due to the viewing angle or a relatively smooth stellar distribution. Possible signs of minor tidal disturbances are visible, without any signs of major mergers or interactions. 
