The galaxy presents as a relatively smooth, elliptical structure. Its shape is moderately elongated, appearing somewhat cigar-shaped. The central region exhibits a brighter, more concentrated luminosity, indicating a higher density of stars. There is a subtle color gradient, with the core appearing slightly more yellow/white. This suggests an older stellar population in the center. Fainter, bluer regions are observed towards the edges. While the overall structure is smooth, there may be a hint of a faint disk component that lies along the major axis. There is no apparent sign of major merger activity or significant tidal distortions.
