The galaxy presents a generally smooth and featureless appearance. It exhibits an elliptical morphology, appearing somewhat elongated rather than perfectly spherical. The core of the galaxy is bright and exhibits a yellowish hue, likely indicating a population of older stars. Towards the outer regions, a slight blue tint is visible, suggesting the presence of some younger, hotter stars and ongoing star formation, although at a relatively low level. There is no discernible spiral structure or bar. There is no evidence of a major merger, but there could be a minor disturbance. The galaxy appears relatively undisturbed.
