The galaxy appears to be elliptical in shape, presenting a smooth, diffuse light profile. The central region exhibits a higher surface brightness, indicating a concentration of stars and possibly a supermassive black hole. Moving outward from the core, the light intensity gradually decreases, with no distinct spiral arm structures or prominent dust lanes visible. There is a subtle color gradient, with the central regions appearing slightly yellower, which might suggest an older stellar population, and the outer regions presenting a bluer hue, perhaps indicating the presence of younger stars. Overall, the galaxy's appearance is consistent with an early-type galaxy, likely an elliptical, with a relatively quiescent star formation rate. No signs of any major disturbances or mergers are present.
