The galaxy presents as a relatively smooth, centralized structure. It appears elliptical in shape, with a noticeable concentration of light toward the center. The color profile suggests an older stellar population, with a dominant yellowish hue in the core that fades to a slightly redder tone in the outer regions. No distinct spiral arms or significant dust lanes are readily apparent. There may be a slight asymmetry in the outer edges, potentially indicating minor tidal interactions or past mergers, though this is not definitively clear from the presented image. Overall, the galaxy's morphology suggests a system that has largely completed its star formation, with a dominant population of older stars.
