The galaxy presents as a relatively smooth, elongated structure. The central region exhibits a higher concentration of luminosity, appearing nearly spheroidal and with a yellow-white hue, suggesting an older stellar population. Moving outward from the core, the galaxy appears less defined, gradually fading into the background. There is a subtle hint of disk structure, but it's not sharply defined. Minor irregularities are present along the edges of the galaxy. Overall, the system appears to be relatively undisturbed.
