The galaxy presents a primarily elliptical morphology, exhibiting a smooth, largely featureless structure. The central region displays a concentration of light, indicative of a prominent galactic nucleus. The overall color profile suggests a relatively evolved stellar population, with a bias towards older, redder stars, particularly concentrated in the core. No distinct spiral arms or significant dust lanes are readily apparent. The galaxy appears well-defined, possessing a discernible boundary, although the outer edges exhibit a gradual decrease in luminosity. Faint tidal features, if present, are not visibly resolved at this resolution. There is no evidence to suggest that the galaxy is a result of any major merger event.
