The galaxy presents as an elliptical or lenticular type, characterized by a smooth, relatively featureless morphology. Its overall shape is somewhat elongated, deviating slightly from a perfect sphere. The central region exhibits a concentration of light, gradually decreasing in intensity towards the outer edges of the galaxy.

The color profile indicates a population of older stars, with a dominant yellowish-orange hue. The lack of distinct blue regions suggests a relatively low rate of ongoing star formation. There are indications of some tidal disturbance in the form of a faint asymmetry in the outer regions of the galaxy, suggesting past minor interactions, though the galaxy is not currently undergoing a major merger.
