The galaxy presents a generally smooth and centrally concentrated morphology, with a noticeable radial gradient in luminosity. The central region exhibits a bright, yellowish hue, suggesting a concentration of older stellar populations. Moving outward from the core, the light diffuses and the color transitions to a slightly bluer, greenish tint. This suggests the presence of younger stars or nebular emissions in the outer regions, though distinct spiral arms or other features are not clearly discernible. The galaxy's overall structure appears relatively undisturbed, lacking obvious signs of major mergers or significant tidal interactions. However, there may be minor irregularities or subtle disturbances in the outer regions, warranting further investigation. The galaxy's ellipticity appears moderate, indicating it is neither perfectly spherical nor highly elongated.
