The galaxy presents as an elliptical structure with a smooth, largely featureless morphology. It appears to be a relatively concentrated object with a radial distribution of light intensity decreasing from the central region outwards. There is a slight elongation present, suggesting it is not perfectly spherical, but rather somewhat flattened. Color gradients indicate a potentially older stellar population, with the central region exhibiting a yellow-orange hue, suggestive of evolved stars. Fainter bluish hues are present in the outer regions of the galaxy, possibly indicating regions of younger stars at a lower rate of star formation. There is no evidence of significant dust lanes or spiral arm structures. There are no signs of interactions or mergers.
