The galaxy appears to be an elliptical type, with a high degree of central concentration. Its overall form is smooth and rounded. The central region exhibits a bright, yellowish-white color, suggesting an older stellar population dominating the core. Fainter, reddish hues extend outwards from the core, likely indicating a decreasing density of older stars and a possible lower level of ongoing star formation, though it appears quiescent. There is no evidence of spiral arm structure or a prominent disk component, and the galaxy appears relatively undisturbed, without any signs of major mergers or significant tidal interactions. The galaxy's light profile suggests it's a fairly massive system.
