This galaxy presents as an elliptical morphology, characterized by a smooth, centrally concentrated light distribution. The color profile appears generally red, suggesting a population of older stars with lower levels of ongoing star formation. The overall shape is quite round, with no significant elongation or distortions visible. There are no clear signs of spiral arm structures or a prominent disk. Moreover, there is no evidence of any major ongoing mergers or significant tidal disturbances. The system appears to be relatively undisturbed, indicative of a galaxy that has likely undergone significant evolution in isolation.
