The galaxy presents a generally smooth and rounded morphology. Its color profile suggests a dominant population of older stars, exhibiting a reddish hue in the outer regions transitioning to a brighter, yellowish-white core. There is no apparent spiral structure or evidence of a prominent disk. The galaxy appears relatively undisturbed, with no obvious signs of ongoing mergers or tidal interactions. Minor irregularities in the light distribution could indicate faint, unresolved features or subtle internal structures. Overall, the galaxy appears to be a fairly typical early-type system.
