The galaxy presents as a largely featureless elliptical morphology, with a high degree of central concentration. The light distribution appears relatively smooth with a round profile, indicating an absence of prominent spiral arms or a distinct disk structure. There is a subtle elongation observed, suggesting it may be slightly flattened rather than perfectly spherical.

Color gradients within the galaxy suggest a variation in stellar populations. The central region exhibits a yellowish-white hue, potentially indicating a population of older, less massive stars. Fainter, reddish colors are observed at the edges of the galaxy.

The galaxy displays minimal signs of ongoing star formation based on the lack of strong blue colors associated with young, hot stars. Based on these observations, the galaxy can be described as an evolved system with a dominant population of older stars and little to no current star formation activity.
