The galaxy presents a prominent disk-like structure, inclined relative to our line of sight. This orientation complicates precise determination of its morphology, but spiral arm features appear to be present. These arms seem somewhat tightly wound. A central bulge is visible and appears to be of moderate size relative to the disk. There is no obvious bar structure bisecting the bulge. The color distribution suggests a mix of stellar populations, with the bulge exhibiting a yellowish hue, potentially indicating older stars, while bluer colors are present in the disk, suggesting ongoing star formation. No major disturbances or mergers are readily apparent, although minor irregularities might be present in the outer regions of the disk. The overall structure suggests a spiral galaxy in a relatively undisturbed state, with moderate star formation activity.
