The galaxy presents as a relatively compact object. Its morphology appears largely smooth and elliptical, with a high degree of roundness. There is a slight color gradient, appearing bluer in the central region and transitioning to a redder hue towards the outer edges. No prominent spiral arms or distinct features are discernible. There is little evidence of significant ongoing star formation within the galaxy based on the lack of prominent blue or ultraviolet emission regions. Overall, the galaxy gives the visual impression of being a well-evolved system. No interactions or major disturbances are evident.
