The galaxy presents as a moderately compact object with a generally smooth morphology. It appears roughly elliptical in shape, exhibiting a gradual falloff in surface brightness from the center outwards. The core region displays a yellowish-white hue, suggesting a population of older stars. There is little evidence of spiral arm structures or significant dust lanes. Faint hints of bluer light are present in the outer regions, indicating a small presence of younger, hotter stars. The galaxy appears relatively undisturbed, with no obvious signs of tidal interactions or recent mergers. There is no obvious active galactic nuclei or other bright nuclear activity present in the core of the galaxy.
