The galaxy presents as a somewhat elliptical structure, with a smooth, concentrated central bulge that emits strongly in redder wavelengths. This suggests an older stellar population dominating the core region. Moving outward from the core, a fainter, more diffuse halo is observed, exhibiting a subtle color gradient towards bluer hues. This potentially indicates the presence of a younger stellar population and ongoing, though low, star formation activity in the outer regions. The overall morphology shows little evidence of major disturbances or merging events, appearing relatively undisturbed. The galaxy's shape is slightly elongated, not perfectly spherical, with an intermediate axial ratio. There is a subtle hint of a disk component but it is not well defined. The light distribution is generally smooth with few distinct features.
