The galaxy presents a predominantly smooth and elliptical morphology. The central region exhibits a bright, concentrated core, indicative of a substantial stellar population. Moving outward, the galaxy's luminosity gradually diminishes, displaying a diffuse halo. There's a slight elongation, suggesting a deviation from perfect sphericity, possibly exhibiting an oblate spheroidal shape. No distinct spiral arms or prominent dust lanes are visible within the galaxy's structure. A subtle color gradient is observed, transitioning from a yellowish hue at the core to a slightly redder tint in the outer regions. This suggests a possible variation in stellar age or metallicity across the galaxy. There are no visual signs of ongoing major mergers, or significant tidal disturbances in the galaxy's immediate vicinity. It may be undergoing minor disturbances.
