The galaxy presents as a somewhat elongated and diffuse object. It is centrally concentrated, with the luminosity decreasing gradually towards the edges. There is a smooth appearance with a subtle color gradient visible. The central region appears somewhat brighter and more blueish-white, potentially indicating a population of younger, hotter stars. Moving outward, the galactic halo appears more diffuse and red, suggesting an older stellar population. There is no clear evidence of spiral arm structure or a distinct galactic nucleus. The overall morphology is suggestive of a lenticular or possibly an elliptical galaxy.
