The galaxy presents a generally smooth and centrally concentrated appearance. There is evidence of a subtle disk structure, although it is not dominant. The galaxy exhibits a moderate ellipticity, appearing somewhat elongated rather than perfectly spherical. There is no indication of a major merger event in its recent history, although subtle disturbances cannot be ruled out. The galaxy's color gradient suggests a higher concentration of older stellar populations in its central regions, with bluer colors indicating more recent star formation possibly occurring in the outer regions, albeit at a relatively low rate. The galaxy appears to be relatively massive.
