This galaxy appears to be an elliptical galaxy, exhibiting a smooth, centrally concentrated light distribution. The core region is bright, with a yellowish hue suggesting an older stellar population. The light intensity gradually decreases with distance from the center, showing a diffuse halo. There is little to no indication of spiral arms or distinct disk-like structures. Faint irregular features may be present, suggesting a possible minor interaction or recent accretion event, but this is difficult to confirm. Overall, the galaxy appears to be a relatively undisturbed elliptical.
