The galaxy presents a generally smooth, rounded morphology, with a bright, concentrated central region. The light distribution appears relatively uniform, lacking prominent spiral arms or a distinct bar structure. The galaxy exhibits a color gradient, transitioning from bluer hues in the central region to redder tones in the outer regions. This color gradient may indicate a variation in stellar populations, with younger, hotter stars concentrated centrally and older, cooler stars dominating the outer regions. There is some subtle asymmetric distortion that may suggest possible minor tidal disturbance or past interactions. Overall, it appears to be a substantial, relatively evolved system at a considerable distance.
