The galaxy presents as a centrally concentrated object with a smooth, elliptical morphology. There's a discernible radial gradient in luminosity, with the brightest region concentrated at the core, gradually fading toward the outer edges. The galaxy appears to be relatively featureless, lacking prominent spiral arms or distinct dust lanes in this image. The color profile suggests a population of older stars, indicated by the yellowish to reddish hue dominant in the galaxy's body. There is no clear sign of any recent major merging events or significant disturbances in the overall structure. There is a subtle extension of light that may indicate a faint galactic halo surrounding the main body.
