The galaxy exhibits an elliptical morphology, displaying a smooth and centrally concentrated light distribution. The color profile suggests an older stellar population with a dominant yellowish hue, indicative of evolved stars. There is a slight elongation in its overall shape, appearing more oblate than spherical. Faint hints of a disk-like structure may be present, but are not clearly distinguished within the overall smooth profile. No prominent dust lanes or spiral arm structures are apparent. A subtle irregularity can be observed in the outer regions, possibly suggesting minor gravitational interactions or disturbances. 
