The galaxy appears as a relatively small, elongated object. The light distribution is centrally concentrated, with a smooth, diffuse profile lacking distinct spiral arm structures or a prominent bulge. The color is predominantly bluish, suggesting a population of younger, hotter stars. The galaxy exhibits a moderate degree of elongation, appearing somewhat cigar-shaped. There is no obvious evidence of ongoing major mergers or strong tidal disturbances, although some subtle irregularities in the outer regions cannot be ruled out. Based on the overall morphology, this galaxy could be classified as a lenticular or possibly a late-type spiral viewed at a high inclination.
