The galaxy presents as an elliptical or lenticular type with a smooth, centrally concentrated light profile. Its color suggests a moderate amount of star formation, possibly with a mix of older and younger stellar populations. The overall structure appears relatively undisturbed, lacking significant tidal features or evidence of major mergers. There is a subtle color gradient from the inner region to the outer halo, with the core showing a slightly yellower or redder hue compared to the bluer periphery. The galaxy exhibits a nearly circular morphology, with a high degree of roundness. There are no indications of strong spiral arms or prominent disk features; instead, the light is evenly distributed across the galactic body. There may be some minor irregularities or faint features present within the outer regions.
