The galaxy presents a largely smooth morphology, appearing elliptical in shape with a high degree of central concentration. The core exhibits a bright, yellowish-white hue, suggesting a population of older stars. The galaxy's overall form indicates a system that is relatively undisturbed, showing no major signs of ongoing merging activity. The isophotes are generally smooth and well-defined, with a slight elongation hinting at a potential cigar shape. Hints of fainter material extend outwards from the core region. A possible minor disturbance is indicated by a slight asymmetry in the outer regions of the disk. There is a very faint red region at the top side of the galaxy.
