The galaxy presents as a moderately luminous object with a smooth, relatively featureless morphology. Its overall shape appears somewhat elliptical, with a slightly elongated form. The central region exhibits a concentrated, bright core, suggesting a substantial stellar population and potentially a supermassive black hole actively accreting material. The color profile indicates a generally older stellar population, with a yellowish-red hue. There are hints of blue light in some regions. The overall smoothness and lack of distinct spiral arms or irregular structures point towards a galaxy that has likely undergone significant evolutionary processes, potentially involving past mergers or interactions. No significant tidal tails or signs of ongoing major disturbances are visually apparent. The galaxy appears relatively isolated and undisturbed in its immediate environment.
