The galaxy presents a somewhat amorphous structure, exhibiting characteristics of both a smooth elliptical morphology and features suggestive of a disk. The overall form is moderately elongated, leaning toward an "in-between" roundness classification. The light distribution is centrally concentrated but diffuse at the edges, with a noticeable color gradient shifting from a bluer core to redder outer regions. There appears to be some distortion in the galaxy's shape, hinting at possible minor gravitational interactions or internal dynamical disturbances. A portion of the galaxy seems to be undergoing more intense star formation. The overall color suggests a system that has a mix of stellar populations.
