The galaxy presents as a largely smooth, centralized object with a distinct but not perfectly circular morphology. The radial color profile suggests a strong concentration of stellar populations in the galactic nucleus. The overall color is indicative of a mature stellar population, trending towards the redder end of the spectrum, with the central regions appearing more yellow. The overall structure displays no prominent spiral arms or bars, indicating a relatively featureless disk, if one exists. There are no readily apparent signs of active galactic nuclei phenomena or significant dust lanes. There is a hint of some disturbances in the outer edges. The object appears to be relatively isolated, with no obvious signs of ongoing major mergers or tidal interactions with nearby galaxies.
