The galaxy presents as a generally smooth, elliptical-like structure. The core exhibits a concentrated, bright yellow-white luminosity, suggesting a substantial population of older stars. Moving outward from the core, the luminosity diminishes, transitioning to a redder hue, then fading into the background.

The object appears predominantly featureless, lacking any distinct spiral arms or obvious dust lanes within the limits of observational clarity. There may be some minor disturbances in the gradient of light.
