The galaxy presents as a concentrated, smooth object with a generally elliptical morphology. The core exhibits a bright, yellow-white luminosity, suggesting a higher concentration of older stellar populations. Moving outward from the core, the light gradually decreases in intensity, exhibiting a faint reddish color with subtle hints of blue in the outer regions. There is no distinct evidence of spiral arms or prominent dust lanes. The smooth light distribution suggests the galaxy is relatively undisturbed, showing little evidence of recent or ongoing major merger events. The slight elongation may indicate some degree of disk-like structure, but overall the galaxy appears primarily spheroidal.
