The galaxy appears as a centrally concentrated object with a relatively smooth, elliptical morphology. It exhibits a dominant yellowish-orange hue in its central region, suggesting a population of older stars. There is little evidence of distinct spiral arms or significant dust lanes; the overall structure indicates a lack of ongoing major star formation. The galaxy presents a generally rounded shape. There's no sign of any on-going merging activity or major disturbances to its form. The light distribution smoothly diminishes with radial distance from the core.
