The galaxy appears as a diffuse, elliptical structure. Its central region exhibits a brighter, more concentrated luminosity, suggesting a nucleus or a dense concentration of stars. Moving outward from the center, the light gradually fades, creating a soft, extended halo. The galaxy displays a relatively smooth texture, with no immediately apparent spiral arms or prominent dust lanes. There appears to be some asymmetry in the outer regions of the galaxy, hinting at possible tidal interactions or past mergers, although no major disturbances are clearly visible. The overall color of the galaxy appears somewhat redder, indicative of an older stellar population. The galaxy is not perfectly circular but slightly elongated, defining an approximate major axis and minor axis.
