The galaxy appears as a centrally concentrated, relatively smooth object, approximately circular in projection. There is a subtle color gradient, transitioning from a slightly bluer hue in the central region to a redder color towards the outer edges, which suggests a possible difference in stellar populations, with the core possibly containing more younger, bluer stars while the outskirts host older, redder stars. There are no obvious spiral arm structures visible, nor any large-scale disturbances or tidal features, although a very subtle lopsidedness is visible at the lowest surface brightness levels. The galaxy does not exhibit an obvious dust lane or pronounced star-forming regions. The overall morphology points towards a relatively evolved system, likely with a diminished current star formation rate. 
