The galaxy presents as a relatively smooth, centrally concentrated object. It exhibits an elliptical morphology, appearing slightly elongated. The galaxy's light profile suggests a dominant bulge component, with a gradual decrease in luminosity from the core outwards. The color gradient is subtle, with a slightly redder hue in the central region, transitioning to a bluer color in the outer regions. This may indicate a relatively old stellar population within the core, with a younger stellar population distributed in the outer regions. No distinct spiral arm structures or prominent dust lanes are visible. There is no obvious evidence of active galactic nuclei activity or recent major merger events. Overall, the galaxy appears to be a relatively undisturbed system, undergoing moderate levels of star formation.
