The galaxy presents an elongated, somewhat cigar-shaped morphology. A central, bright, yellow-orange bulge dominates the appearance, suggesting a concentration of older stars or dust obscuration. Extending outwards from this bulge are fainter, bluish structures that appear to be spiral arms or tidal features. The overall smoothness indicates it may be an elliptical galaxy in the process of merging. There is no clear indication of active star formation within the bulge, however the blue color of the arms suggest the presence of younger stars. The galaxy exhibits some signs of disturbance, potentially due to a minor gravitational interaction. The estimated size is roughly 12.5 kpc.
