This galaxy appears as a centrally concentrated object with a relatively smooth morphology. The core is bright and concentrated, exhibiting a near-spherical symmetry. A faint, diffuse halo surrounds the central region, with subtle extensions. There is a slight asymmetry to the outer edges, possibly indicating minor tidal disturbances or interactions. Color gradients are noticeable, with a bluer hue in the inner regions, suggestive of younger stellar populations or enhanced star formation, and a shift towards redder tones further from the center, possibly indicative of older, cooler stellar populations. There is no distinct spiral structure or bar visible. The overall structure is dominated by a smooth distribution of light. The galaxy is relatively compact. The visual characteristics suggest a system that might have undergone minor merger events or experienced some form of morphological transformation.
