The galaxy presents a generally smooth and elliptical morphology. The core is a bright, concentrated region that appears relatively spheroidal. There is a discernible gradient in light intensity, with luminosity decreasing steadily from the center outwards. While a distinct disk is not evident, there may be some faint and diffuse features or irregularities along the edges, but they are subtle and difficult to resolve clearly. Overall, the galaxy exhibits a degree of symmetry with no strong evidence of ongoing major mergers or tidal disturbances. There is no concentrated blueness indicative of a young stellar population, suggesting a possible lack of significant current star formation. The galaxy likely hosts a mature stellar population.
