The galaxy presents as an elliptical morphology, elongated in shape with a high degree of smoothness. A distinct central bulge is visible, exhibiting a concentration of light, likely indicating a high stellar density. The overall color gradient shifts from a bluer periphery to a redder core, suggesting a population of older stars concentrated within the central region. No discernible spiral arms or prominent dust lanes are observed. Minor asymmetry and slight disturbances are hinted at in the outer regions, potentially suggesting past minor interaction or merging event.
