The galaxy presents an elliptical morphology. Its core exhibits a bright, concentrated luminosity, transitioning outwards to a less defined, fainter halo. The color profile indicates a predominantly older stellar population, as evidenced by the reddish-yellow hue concentrated in the central bulge, potentially indicating a high concentration of evolved red giant stars. There is a slight asymmetry in the outer regions, suggesting a possible minor interaction or tidal disturbance, however the overall structure appears relatively smooth and undisturbed. No prominent spiral arm structures are observed.
