The galaxy presents as an elliptical morphology, with a generally smooth texture. The color profile appears relatively uniform throughout, with a dominant bluish-white hue in the central region that may indicate some ongoing star formation, though it is likely at a low rate. The outer regions of the galaxy become more diffuse and less defined, indicating a gradual decrease in stellar density. There is no apparent evidence of spiral arm structures, dust lanes, or a prominent galactic nucleus. The overall shape appears somewhere between round and elongated with no signs of major disturbances in its form, though there may be a slight asymmetry or minor irregularity in the outer halo.
