The galaxy presents as a relatively smooth, elliptical-like structure, with a central, bright bulge. The color distribution appears somewhat uniform, tending towards warmer hues in the optical spectrum, suggestive of an older stellar population. There's little indication of spiral arm structure or significant dust lanes. The overall morphology is largely undisturbed, showing no obvious signs of recent major mergers or tidal interactions. There might be some minor asymmetry in the outer regions, possibly indicating subtle disturbances, but these features are not strongly pronounced.
