The galaxy presents as a fairly smooth, elliptical morphology. There is an apparent lack of distinct spiral arms or a well-defined disk structure. The light distribution appears concentrated towards the center, indicative of a prominent bulge. It appears to be a redder galaxy, showing primarily in the redder bandpasses. The color suggests an older stellar population. The galaxy appears elongated, deviating slightly from a perfectly circular shape. There is no evidence of ongoing major mergers or significant tidal disturbances from this image alone, although a minor interaction cannot be ruled out.
