The galaxy presents as a somewhat elliptical, lens-shaped object. Its core is a bright, concentrated yellow hue, suggesting a population of older stars and/or dust obscuration. Fainter disk-like arms emanate from the core. The arms are quite smooth, not flocculent in nature, suggesting a relatively ordered structure without strong disturbances. There are hints of blue light within the disk, possibly indicating regions of more recent star formation. No spiral structure is immediately visible. The galaxy is not highly inclined. There is no obvious evidence of a major ongoing merger. The object appears relatively isolated, with no nearby companions that could be gravitationally interacting with it. Overall, it seems to be an intermediate luminosity disk galaxy, likely with a significant bulge component.
