The galaxy presents a largely featureless, smooth morphology. It is dominated by a central, bright bulge that gradually fades outward into a more diffuse halo. The galaxy appears elliptical in shape, exhibiting a high degree of roundness. There is no discernible spiral arm structure or prominent dust lanes. A subtle color gradient is observable, with the central bulge exhibiting a slightly redder hue compared to the outer regions. No evidence of any major disturbances, tidal tails, or merging companions is apparent. The galaxy exhibits low star formation, suggesting an older stellar population.
