The galaxy presents as a centrally concentrated object with a generally smooth morphology. There is a bright central bulge that appears roughly spherical, surrounded by a fainter, more diffuse halo. The overall shape is somewhat elongated, suggestive of a mild ellipsoidal structure, however, it is difficult to make out distinct structural features such as spiral arms or a well-defined disk component. The color distribution suggests a stellar population with a significant fraction of older stars. A slight color gradient is present, with the central region exhibiting a yellower, possibly redder, hue. The outer halo is slightly bluer in comparison, indicating the potential presence of younger stars or perhaps ongoing, although subdued, star formation activity. The image does not show evidence of major mergers or significant tidal disturbances, however, there may be minor asymmetries in the outer regions hinting at possible past interactions. Overall, the galaxy appears to be a relatively massive system with a dominant bulge and a quiescent star formation rate.
