The galaxy appears to be an elliptical galaxy, exhibiting a smooth, centrally concentrated light distribution. The galaxy's shape is generally round, showing minimal deviation from circularity. The central region is bright, gradually fading into the outer regions. There are no prominent spiral arms or distinct disk features visible. Color gradients are subtle, with a yellowish-white core transitioning to a slightly redder halo. There is no obvious evidence of ongoing major mergers or significant tidal disturbances; however, there may be some minor irregular features present that could indicate some interaction. Overall, the galaxy presents a relatively relaxed morphology, consistent with an evolved stellar population.
