The galaxy presents as a centrally concentrated object with a generally smooth morphology. Its shape is elliptical, approaching a more rounded form with a slight elongation. The core region appears bright and concentrated with a yellowish hue, suggesting a population of older stars. Moving outwards from the core, the galaxy transitions to a fainter, more diffuse halo with a slightly redder color, which indicates either an older stellar population or dust obscuration. There is a hint of some minor structural disturbance within the outer regions, but overall, it is dominated by smooth light distribution. There is no visible spiral arm structure or signs of active star formation.
