The galaxy presents a predominantly smooth morphology, with a centrally concentrated luminosity profile. It appears roughly elliptical in shape, exhibiting a high degree of roundness. There is a lack of pronounced spiral arm structure or significant dust lanes visible in this imagery, suggestive of an earlier-type classification. Hints of a fainter, diffuse halo may be present, surrounding the brighter central region. The color profile indicates a potential population of older stars, with some regions appearing bluer. The overall structure appears relatively undisturbed, displaying no obvious signs of major recent mergers.
