The galaxy presents as a relatively smooth, elliptical morphology. Its overall shape appears elongated, but not significantly distorted. The central region exhibits a strong concentration of light, appearing much brighter than the outer regions, which fade gradually. There may be the slightest hint of disk like structure, though it appears subdued and not particularly well-defined. There is little evidence of prominent spiral arms or substantial dust lanes. Color gradients suggest an older stellar population, as indicated by the yellow to red hue of the central bulge. The overall structure indicates a system nearing quiescence, with a moderate mass. It seems to be undergoing a relatively low level of star formation.
