The galaxy presents a generally elliptical morphology with a smooth light distribution. There is a distinct central bulge that exhibits a bright, concentrated luminosity. Moving outward from the center, the light gradually fades into a diffuse halo or disk-like structure. There appears to be very little resolved structure within the galaxy, such as prominent spiral arms or distinct dust lanes. There may be some minor irregularity within the halo region, though it's hard to tell if this is merely due to image noise. The overall color appears to be slightly reddish-yellow, indicative of an older stellar population. The galaxy shows no clear signs of a major merger or tidal disruption.
