The galaxy presents as a relatively smooth, elliptical morphology. It exhibits a central bulge that is moderately bright with a slightly reddish hue, surrounded by a more diffuse halo. The overall shape appears close to circular with minimal discernible disc structure or spiral arms. There is some indication of minor disturbance in the outer regions, though the galaxy does not appear to be undergoing a major merger. The light distribution is concentrated towards the center, suggesting a relatively old stellar population, yet there is still indication of some star formation. Overall, the galaxy appears to be a fairly evolved system with characteristics somewhere between a spiral and a lenticular galaxy.
