The galaxy presents as a centrally concentrated object, exhibiting a flattened, elliptical morphology. A smooth, diffuse halo surrounds a brighter, more compact core. The central region displays a yellow-orange hue, possibly indicative of an older stellar population. The outer regions of the galaxy are less defined, with a gradual decrease in luminosity towards the edges. A slight blue tint is observed within the halo of the galaxy. The overall structure suggests a relatively evolved galaxy, with limited evidence of spiral arm structure or active star formation in the core. The luminosity profile appears to be centrally peaked, and the size suggests a moderately large object. There is some distortion in the shape of the galaxy, indicating some possible tidal disruption.
