The galaxy presents as a relatively smooth, elliptical-like structure. A bright, concentrated nucleus is visually apparent, surrounded by a less defined, more diffuse halo of light. Faint blue hues are observed in what could be loosely described as a disk or extended feature beyond the nucleus, suggesting the presence of younger stellar populations and ongoing star formation. The galaxy appears to be experiencing only minor gravitational disturbances, with subtle asymmetrical features perhaps indicating a small tidal interaction. Overall, the galaxy's morphology suggests a transition between a pure elliptical and a more disk-like structure.
