The galaxy presents a generally smooth, elliptical morphology. Its central region exhibits a concentrated, bright, yellowish-white core, suggesting an older stellar population dominates. The galaxy appears moderately compact, with an estimated effective radius spanning roughly 10 kiloparsecs. The outer regions show a gradual decrease in luminosity and a slight bluish tint, potentially indicating a younger, though subdued, population of stars in the outskirts. There are no distinct features, such as spiral arms or prominent dust lanes, discernible in this image. The overall structure suggests a relatively relaxed system, possibly nearing the end-stage of its evolution with a moderate star formation rate. No signs of significant tidal disturbances or major ongoing mergers are apparent.
