The galaxy appears as a lenticular, disk-shaped system, exhibiting a smooth, elliptical morphology. The central bulge is prominent and concentrated, displaying a yellowish-orange hue, suggestive of an older stellar population. Moving outward from the core, the disk exhibits a flattening, with the color gradually transitioning to a more diffuse, bluish tint. There are weak hints of spiral arm structures in the periphery, but these are not well-defined. The galaxy's overall shape is somewhat elongated, displaying a cigar-like form, possibly indicating it is in the process of merging with another galaxy, although there are no clear signs of major disturbances. Based on the apparent colors and morphology, this galaxy is classified as an early-type spiral with little observable star formation.
