The galaxy presents an elliptical morphology, exhibiting a smooth light distribution. The core region displays a concentrated, bright glow with a yellowish hue, indicative of an older stellar population. Moving outwards from the core, there is a subtle decrease in the yellow light and a transition to a faint greenish color, suggesting the presence of some younger stars or ionized gas, albeit minimal. The outer edges of the galaxy gradually fade into the background, showing no distinct spiral arm structures or prominent dust lanes. Overall, the galaxy appears to be relatively undisturbed with no signs of ongoing major mergers or tidal distortions. It presents as a mature system with a dominant, well-established spheroidal component.
