The galaxy presents as a centrally concentrated, smooth object, with a subtle, elongated morphology. Its color profile exhibits a dominant yellowish-white hue in the core, suggesting a population of older stars. Fainter bluish tints are present in the outer regions, possibly indicating the presence of younger stars. No distinct spiral arm structures or prominent dust lanes are discernible. The galaxy exhibits a moderately compact size, with an overall smooth luminosity gradient from core to edge. There are no obvious signs of active galactic nuclei activity or ongoing major merger events. The system appears generally undisturbed.
