The galaxy presents as a somewhat disrupted spiral, possibly an intermediate type. The central bulge is prominent and appears relatively smooth and spheroidal. The surrounding disk shows evidence of spiral arms, though they are not particularly well-defined or symmetrical. One arm appears to be more defined, while another is more distorted, and possibly merging or interacting with another galaxy. The galaxy has a moderate inclination relative to our line of sight. The color gradients across the galaxy suggest varying stellar populations, with a slightly bluer disk and redder central bulge. Faint tidal features are apparent, which is consistent with recent or ongoing merger activity.
