The galaxy presents as a generally smooth, centrally concentrated object with a somewhat round morphology. The light profile appears to decrease gradually from the bright core outwards. There is some evidence of faint, diffuse, extended emission surrounding the core, but no distinct spiral arms or bar structures are discernible in the image. The color appears relatively uniform across the galaxy, with a yellow-white hue indicative of an older stellar population. There is some suggestion of minor disturbances, but no clear signs of major merging activity or tidal tails are apparent.
