The galaxy presents as a relatively compact, elliptical-like structure, with a dominant central bulge. The light distribution appears smooth and concentrated. There is a pronounced color gradient, transitioning from a yellowish-orange core to a slightly bluer outer region. The galaxy does not show any obvious signs of strong spiral arms or a well-defined disk. The overall morphology suggests a system dominated by an older stellar population, though some ongoing star formation cannot be ruled out in the outer regions. There is no clear indication of any major ongoing merger events, however, there is some indication of minor disturbances, and some asymmetry in the outer regions.
