The galaxy presents an overall elliptical morphology, with a moderate axis ratio. The light distribution appears relatively smooth and centrally concentrated, with a bright, diffuse core. The color profile suggests a population of older stars, indicated by the yellowish-red hue dominating the galaxy's central region. There's a subtle color gradient, transitioning towards slightly bluer tones in the outer regions, hinting at the presence of a younger stellar population or ongoing star formation, albeit at a low rate. There are no prominent spiral arms or dust lanes visible. There appears to be a slight tidal disturbance feature on the edge of the galaxy, though this is not clearly defined.
