The galaxy appears as a relatively smooth, elliptical-like structure. The light profile seems to be centrally concentrated, with a gradual falloff in intensity towards the outer regions. The color is generally consistent across the galaxy, trending towards a redder hue. There is no apparent spiral arm structure or significant dust lane obscuration visible. Based on the smoothness and color profile, it is likely that this galaxy is composed primarily of older stellar populations. The overall morphology suggests a galaxy that has undergone significant evolution, potentially through mergers or secular processes, leading to the present smooth, red appearance. There are no obvious signs of active star formation regions.
