The galaxy presents as a relatively smooth, elliptical-like structure. Its overall color is a yellowish-white, suggesting a population of older stars. There is a brighter, more concentrated core region. The galaxy appears somewhat round, lacking any obvious spiral arm features or strong bar structures. There is subtle asymmetry, possibly indicating a minor disturbance or past interaction. A faint halo surrounds the central region, gradually fading into the background. The overall morphology suggests a galaxy towards the earlier end of the Hubble sequence.
