The galaxy presents as a relatively smooth, elliptical structure. The core region exhibits a bright, concentrated luminosity, suggesting a high density of stars. Moving outwards from the core, the light gradually diffuses, forming a somewhat indistinct halo or envelope around the central region. There is a slight elongation in its shape, hinting at an elliptical morphology that is neither perfectly spherical nor highly flattened. The overall color profile appears to lean towards a yellowish-white, potentially indicative of an older stellar population dominating the light output, with a subtle hint of blue, which could denote a minor amount of recent star formation. No distinct spiral arms or prominent dust lanes are visible within the resolution of the image. Overall, it appears to be a galaxy with a relatively quiescent star formation rate.
