The galaxy presents an elliptical morphology, displaying a smooth, featureless structure indicative of a relatively evolved system. Its overall shape approximates a prolate spheroid, appearing elongated but without a distinct disk. The central region exhibits a brighter, concentrated luminosity, suggesting the presence of a prominent galactic nucleus. A subtle color gradient can be observed, with the core exhibiting a yellowish-red hue, potentially implying a population of older, cooler stars. The outer regions of the galaxy appear slightly bluer, which could indicate a minor presence of younger stars or ongoing, albeit subdued, star formation activity within the galaxy's outer reaches. There is no evidence of spiral arms, bars, or any significant tidal distortions that might suggest a recent merger event. The galaxy appears relatively isolated and unperturbed.
