The galaxy presents a primarily smooth morphology, lacking any distinct spiral arms or bar structures. The light distribution appears centrally concentrated, with a gradual decrease in surface brightness towards the outer regions. The overall shape is largely elliptical and somewhat roundish. The color profile indicates a predominantly older stellar population, characterized by yellowish hues, especially concentrated in the center. The presence of some bluer regions suggests more recent star formation. There's a possible hint of minor disturbances in the galaxy's structure, such as a subtle asymmetry or faint tidal features that could indicate past interactions or mergers. Based on the color indices, this galaxy is a relatively massive system. It's likely a well-established galaxy that has ceased most of its star formation and is approaching a quiescent state.
