The galaxy presents a largely smooth, elliptical morphology. It exhibits a concentrated central bulge, which appears yellowish in color, suggesting an older stellar population. The galaxy is moderately elongated, with a subtle disk-like structure. The outer regions of the galaxy fade gradually, without any distinct edges, indicating a halo of stars extending beyond the main body. There is a hint of a very faint spiral structure, but it is difficult to discern from the image. No major disturbances or ongoing mergers are readily apparent, though there is a slight asymmetry on the left side of the galaxy, suggesting a minor interaction in the past. Overall, the galaxy appears to be relatively quiescent with low levels of star formation. 
