This galaxy presents as an elliptical morphology, with a relatively smooth light distribution. The central region exhibits a high concentration of light, suggestive of an older stellar population, potentially with a supermassive black hole at its core. Moving outwards from the center, the light gradually diminishes, forming a diffuse halo. There's a subtle color gradient visible, with the core exhibiting a yellowish hue, possibly indicating a greater abundance of older, redder stars and the outer regions have a faint blue color. There is little evidence of spiral arms or significant dust lanes within the galaxy's structure. Overall, the galaxy appears to be in a relatively quiescent state, lacking prominent features of active star formation.
