The galaxy presents a somewhat elliptical morphology, appearing elongated rather than perfectly spherical. The central region exhibits a high degree of smoothness and a brighter, more concentrated light distribution, likely indicating a significant stellar bulge. Moving outwards from the core, a fainter, more diffuse disk-like structure is visible. Subtle features are present within this disk, but do not give a clear spiral structure. The galaxy displays a color gradient, transitioning from a reddish hue in the central bulge to a slightly bluer color in the outer disk. This color difference suggests a variation in stellar populations, with older, redder stars dominating the bulge and younger, bluer stars present in the disk where star formation may be ongoing. There may be some minor disturbances in the outer regions, hinting at potential interactions or past mergers.
