The galaxy appears to be a relatively smooth, elliptical galaxy, displaying a generally rounded morphology. The central region exhibits a strong concentration of light, indicating a prominent galactic nucleus or bulge. The color profile suggests a population of older stars, with a yellowish hue dominating the core, transitioning to redder colors in the outer regions. There is minimal evidence of spiral arm structure or significant dust lanes. Faint indications of disturbances may be present in the outskirts, though this is subtle and could be due to imaging artifacts. The overall impression is of a quiescent, evolved galaxy, with little active star formation.
