The galaxy presents an overall elliptical morphology with a notable bulge. The light distribution indicates a relatively smooth structure, suggesting a lack of prominent spiral arms. Color gradients are visible, with a yellowish central region that may indicate an older stellar population in the bulge. Moving outwards from the center, the galaxy fades into a bluer hue possibly pointing to younger stars present in the surrounding areas. The ellipticity of the galaxy is noticeable. There seems to be a faint tidal tail on one side of the galaxy, possibly a result of a past minor interaction. The galaxy is not perfectly smooth; close inspection reveals some degree of disturbance within its structure. Overall, the galaxy appears to be in a relatively evolved state.
