The galaxy presents as an elliptical morphology, with a smooth, centrally concentrated luminosity profile. The core exhibits a yellowish hue, suggesting a population of older stars. The isophotes are generally regular and elliptical in shape, but with subtle deviations from perfect ellipticity; the galaxy appears slightly elongated. There is no apparent spiral arm structure, dust lane obscuration, or prominent star-forming regions visible in the image. The overall color gradient from the core outward suggests a decreasing mean stellar age. The image does not show any signs of major recent merger activity, tidal tails, or other significant disturbances to its structure. Faint, diffuse bluer regions are also observed in the outer parts of the galaxy, potentially indicating traces of past interaction or residual low-level star formation.
