The galaxy presents a largely smooth, elliptical morphology, with a high degree of central concentration. It appears generally round in shape. The color profile suggests a dominant population of older stars, as indicated by the redder hues towards the galactic center. There is a subtle color gradient, transitioning towards bluer tones in the outer regions, potentially indicating some ongoing, albeit low, level of star formation in the periphery. There is no distinct spiral arm structure or prominent dust lanes visible, suggesting a relatively quiescent galaxy with limited recent merger activity. There are slight distortions in the galaxy's shape, and the merging data shows some minor disturbance. The overall impression is of a mature galaxy with a relatively smooth and evolved stellar population.
