The galaxy presents as a centrally concentrated object with an elliptical morphology. It exhibits a relatively smooth light distribution, with no distinct spiral arms or other sharp features readily apparent. The galaxy's core displays a bright, yellowish hue, indicative of an older stellar population. The outer regions exhibit a bluer tint, potentially signifying some level of ongoing, though subdued, star formation. There are hints of tidal disturbances, perhaps due to a minor disturbance or past interaction. Overall, this galaxy appears to be in a relatively advanced stage of its evolution, with a dominant spheroidal component.
