The galaxy appears to be elliptical, with a smooth, round morphology. There is no discernible disk structure or spiral arms. The central region exhibits a higher concentration of light, indicating a possible bulge or core. Color gradients suggest a possible variation in stellar populations, with a central region that appears more yellow. There is no indication of major disturbances or mergers. The galaxy appears relatively isolated, with no nearby interacting companions visible in the immediate field.
