The galaxy presents as a relatively smooth, elliptical-like structure with a concentrated central bulge. The light distribution appears centrally peaked, with a gradual decrease in intensity moving outwards from the core. The core region exhibits a yellowish hue, suggesting an older stellar population, while the outer regions have a slightly bluer tint, possibly indicating a younger stellar population. There's no strong indication of spiral arms or prominent disk-like features. There is only minor disturbance to the galaxy, it appears to be relatively undisturbed.
