The galaxy presents a largely smooth morphology, exhibiting a centrally concentrated light distribution. The core region displays a prominent yellowish hue, suggesting a population of older stars and/or dust obscuration. Moving outward from the core, a gradual transition to a more greenish coloration is observed. The outer regions show less definition, fading smoothly into the background sky. Overall, the galaxy appears to be elliptical in shape, lacking any apparent spiral arm structures. There is no obvious evidence of significant tidal disturbances or recent merger activity, though a very slight asymmetry cannot be entirely ruled out.
