The galaxy presents a disk-like structure that is slightly inclined relative to our line of sight. Spiral arms are apparent, although somewhat patchy and not as clearly defined. The galaxy has a prominent central bulge that seems moderately sized, with a bright yellow hue, potentially indicating a significant population of older stars. The disk portion of the galaxy exhibits a bluer color, hinting at ongoing star formation. There are faint traces of what could be tidal disturbances or interactions, suggesting past or ongoing minor mergers.
