The galaxy presents as a generally smooth, centrally concentrated object, with an elliptical morphology. The core exhibits a bright, concentrated luminosity, suggesting a high stellar density. Progressing outwards from the core, the light gradually diminishes, and there is a diffuse halo. Overall, there appears to be a lack of prominent disk features or spiral arms. The color profile suggests a relatively evolved stellar population, as evidenced by the redder hues. There is a possible slight disturbance of the structure on one side, but overall the galaxy presents a relatively unperturbed system.
