The galaxy presents as an elliptical morphology, with a relatively smooth, featureless appearance in the observed optical wavelengths. The light distribution is concentrated towards the center, indicative of a prominent galactic bulge.  The core exhibits a yellowish-orange hue, suggesting a population of older stars. The outer regions show a slight decrease in intensity, with hints of greenish tones. The galaxy displays a slight disturbance with the possibility of being in the minor process of merging with a nearby object. This object is not easily determined due to its small size and faintness. Overall, the galaxy appears to be evolved, quiescent, with low star formation activity.
