The galaxy appears to be a relatively smooth, elliptical type. It exhibits a concentrated central bulge, with a gradual decrease in luminosity towards the outer regions. The color profile indicates a redder core, possibly due to an older stellar population or dust obscuration. There's a hint of a disk-like structure but it isn't very prominent. It doesn't appear to be undergoing any major merging activity, though there may be minor disturbances in its structure. Overall, the galaxy seems relatively undisturbed.
