The galaxy presents a generally smooth and concentrated morphology. There is an apparent central bulge, exhibiting a yellowish hue, suggestive of an older stellar population. Surrounding the bulge, a fainter, more diffuse halo is observed. The overall shape appears elliptical to somewhat in between elliptical and disk-shaped. There is no clear evidence of strong spiral arm structure or a prominent disk component. Faint disturbances or asymmetries might be present in the outer regions, though this is difficult to ascertain. Based on the color profile and morphology, this galaxy likely has moderate to high mass with an ongoing rate of star formation.
