The galaxy presents as a centrally concentrated object with an elliptical morphology. The core exhibits a bright, yellowish-white luminosity, suggesting a population of older stars. Moving outward from the core, the light gradually fades into a reddish hue, especially in the outer regions. The overall smoothness of the light distribution indicates a lack of distinct spiral arms or features. There may be a faint disc-like structure faintly visible in the lower part of the galaxy. There are no signs of any major ongoing merger events or strong tidal disturbances. The galaxy appears to be a relatively undisturbed system, dominated by an older stellar population.
