The galaxy presents as a centrally concentrated object with a generally smooth morphology. It appears largely featureless, lacking discernible spiral arms or a prominent disk structure. Its shape is approximately elliptical, with some elongation. The light distribution is relatively uniform, showing a gradual decrease in intensity from the core outwards. The core exhibits a yellow-white hue, potentially indicating an older stellar population, and the colors become slightly redder in the outer regions. There is no strong evidence of ongoing star formation or significant dust lanes within the galaxy based on visible colors and features. There are no nearby galaxies with which it appears to be interacting.
