The galaxy presents as a relatively smooth, elliptical-like structure. Its overall color is yellowish-orange, which could indicate an older stellar population. There is a brighter central region, possibly a galactic bulge, which graduates into a fainter, more diffuse halo. The galaxy has a slight elongation, deviating from a perfectly circular shape. Evidence of spiral arms or significant dust lanes is absent based on the image. There is no strong sign of any major ongoing mergers or tidal disturbances, suggesting the galaxy is relatively isolated and undisturbed.
