The galaxy presents an overall elliptical morphology. The central bulge exhibits a smooth, diffuse appearance with a concentrated luminosity gradient. Proceeding outward from the bulge, a faint disk component can be discerned; this disk appears somewhat disturbed and asymmetric. The galaxy displays a yellow-orange hue, indicating an older stellar population, while hints of bluer regions suggest ongoing star formation. There is a slight indication of tidal features or minor disturbance within the galaxy's outer regions, which may be indicative of past or ongoing interactions.
