The galaxy exhibits a generally elliptical morphology, with a bright, concentrated central bulge. There is evidence of a flattened disk component surrounding the bulge, though the disk appears relatively smooth with only subtle features. The color gradients suggest a population of older stars dominating the bulge, trending toward slightly bluer colors in the disk, which hints at ongoing, though perhaps subdued, star formation activity. There is a noticeable but mild disturbance to the morphology of the galactic core, which has a knot of blue light, suggesting that a minor merger or tidal interaction could have occured, but it is currently a relatively relaxed system. The overall structure does not display strong spiral arm features. The outer regions of the galaxy appear diffuse and fade gradually into the background sky.
