The galaxy presents as a disk-shaped morphology, viewed at an oblique angle. The central region exhibits a concentrated luminosity, appearing yellow-white in color, potentially indicative of an older stellar population. The outer disk shows a subtle gradient in color, transitioning towards a redder hue. This may reflect differences in stellar populations and dust distribution within the galaxy's structure. There is a fainter object in the same field of view, but there is no clear evidence of a major merger event within the system. The galaxy appears relatively undisturbed.
