The galaxy presents a disk-like morphology, viewed at a significant inclination. The central region exhibits a bright, concentrated nucleus with a slightly reddish hue. Surrounding this is a more extended, but still relatively smooth, bulge component. The disk is composed of several distinct features. There are what appear to be bright knots, indicating regions of active star formation. These regions appear more pronounced on one side of the galaxy than the other, possibly indicating asymmetry in the star formation rate or dust distribution.

The overall color profile suggests a mix of stellar populations. The redder core likely houses older stars, whereas the bluer disk and knots correspond to younger, hotter stars forming within the spiral arms. Evident tidal features suggest this galaxy has undergone a merging event. Some of these features are less distinct but it is clear there is ongoing galactic interaction with another galaxy.
