The galaxy presents as a relatively smooth, centrally concentrated object. Its morphology appears largely spheroidal, with a high degree of roundness and negligible deviation from axial symmetry. There is no distinct disk component or spiral arm structure visible. The galaxy exhibits a luminosity profile that peaks sharply at the center, gradually decreasing towards the outer regions. Color gradients suggest that the central regions of the galaxy are generally yellower than the outer regions. There is no evidence of any significant ongoing merger activity or major tidal disturbances influencing the galaxy's structure. Faint extensions may be present.
