The galaxy presents as a generally smooth, elliptical-like structure. Its core exhibits a concentrated, bright emission, with a gradual decline in luminosity moving outwards. There is a slight elongation, deviating from a perfect circular form. The central region displays a yellowish hue. Fainter extensions are visible, showing a bluer tint. There is no clear evidence of spiral arms, but the disk-like appearance is present. The system appears relatively undisturbed, showing no significant signs of a major merger event. Overall, the galaxy seems to be undergoing relatively low levels of star formation activity.
