The galaxy presents as a slightly elongated spheroid with a dominant central bulge. The color profile suggests an older stellar population in the core, indicated by the yellow-orange hue, likely consisting of Population II stars. The outer regions appear bluer, suggesting more recent star formation activity and the presence of younger, hotter Population I stars. There appears to be some irregular structure within the galactic disk. There is a potential hint of spiral arm structure, but this is hard to tell due to limited detail in the image. There is no evidence of a strong tidal interaction or ongoing major merger, although subtle morphological disturbances could be present. The galaxy exhibits characteristics of both elliptical and spiral galaxies.