The galaxy presents as a relatively smooth, elliptical-like object, exhibiting a centrally concentrated light distribution. A distinct, reddish core region is apparent, suggesting an older stellar population and possibly a supermassive black hole at the center. The outer regions display a more diffuse, greenish glow, possibly indicative of some ongoing star formation, albeit at a lower rate compared to actively star-forming galaxies. No prominent spiral arms or strong dust lanes are discernible. There appears to be a minor disturbance in its shape, possibly from a past or ongoing minor merger event. Overall, the galaxy seems to be in a relatively evolved state, exhibiting characteristics of a transitioning or quiescent system.
