The galaxy presents a relatively smooth morphology, appearing as a centrally concentrated object. There are indications of a disk-like structure, though it is not sharply defined. The central region exhibits a brighter, more condensed core, surrounded by a fainter, extended halo or envelope. Patches of bluer color appear outside of the core, suggesting regions of more recent star formation, although the overall color is moderately red. The system shows no strong signs of major mergers or tidal disturbances, though subtle asymmetries or minor disturbances may be present. The galaxy is not perfectly symmetrical, hinting at some internal dynamics or past interactions, though the dominant impression is that of a well-established, relatively quiescent system.
