The galaxy presents as a relatively smooth and elliptical morphology. The light is concentrated towards the center, with a gradual decrease in brightness as one moves outward. The core appears bright and slightly yellow, indicating a potentially older stellar population. There's a subtle color gradient, with the outer regions exhibiting a slightly bluer hue, hinting at the presence of younger stars, though not as pronounced as in spiral galaxies. No distinct spiral arms or prominent dust lanes are visible. There may be some minor irregularities or disturbances in its structure, but overall, it appears to be a well-formed galaxy in a relatively stable state.
