The galaxy presents as an elliptical morphology, exhibiting a smooth, featureless structure. The light distribution is centrally concentrated with a gradual decline in intensity towards the outer regions. The overall color appears to be a yellow-orange hue, suggesting an older stellar population, potentially dominated by evolved stars. There is a slight elongation visible, deviating from a perfectly circular shape. No prominent dust lanes, spiral arms, or active star-forming regions are clearly discernible. There is a hint of disturbance, but there is nothing to suggest the galaxy is undergoing a major merger or tidal disruption. The galaxy looks to be relatively undisturbed.
