This galaxy appears to be a relatively smooth, elliptical system. The light is concentrated towards the center, with a noticeable decrease in intensity moving outwards. The core exhibits a yellowish hue, suggestive of an older stellar population. There is a very faint, diffuse outer region where some faint disk-like components may be present, however the general shape is very smooth and spheroidal, consistent with an elliptical morphology. There is no clear evidence of spiral arms or a distinct dust lane. There are no obvious signs of a major ongoing merger, although some minor disturbances cannot be ruled out. Overall, this galaxy is consistent with a spheroidal system with moderate mass and a low star formation rate.
