The galaxy appears as a singular, relatively smooth object with a concentrated central bulge. The light distribution exhibits a spheroidal morphology, lacking any prominent spiral arms or bar structures. The color profile suggests an older stellar population, with a dominant yellowish-orange hue, indicative of evolved stars. The galaxy appears to be relatively undisturbed, exhibiting no clear signs of ongoing major merger activity or tidal interactions. It presents a largely elliptical shape, leaning towards being mostly rounded with little elongation. There seems to be minimal disk structure, which could suggest that star formation activity is relatively low.
