This galaxy presents as a relatively smooth, elliptical structure. The core appears luminous, with a yellowish-white hue indicating an older stellar population. The galaxy exhibits a slight elongation, deviating from a perfectly circular form. A faint, diffuse disk-like structure surrounds the central bulge, contributing to a fuzzy outer region. There is a subtle color gradient from the core outwards, with the outer regions appearing slightly bluer, hinting at the presence of some younger stars, or the effects of dust. No significant tidal features or signs of major mergers are apparent. The overall morphology suggests a galaxy that is either evolving passively or experiencing a period of relatively low star formation.
