The galaxy presents as a somewhat diffuse, elliptical-like structure. It exhibits a concentration of light toward its core. The core region appears yellowish, potentially indicating an older stellar population or significant dust extinction. The outer regions of the galaxy fade gradually, showing a reddish hue. This redder color in the outer regions could be due to a population of older, redder stars and/or dust reddening effects. There is a secondary concentration of light beneath the brighter center. Overall, the galaxy appears relatively smooth, with no prominent spiral arms or distinct features readily discernible in this image. There appears to be no major ongoing interaction with other galaxies. The shape is mostly round. There is a chance this is a merger.
