The galaxy presents as a central, moderately luminous object with a smooth, elliptical morphology. It exhibits a concentration of light toward the center, suggesting a significant bulge component. The galaxy appears largely featureless, with no obvious spiral arm structures or dust lanes visible in this imaging. It presents a color profile generally consistent with an older stellar population, dominated by redder wavelengths, though there is evidence of some bluer emission as well. There is no indication of significant ongoing merger activity.
