The galaxy presents as an edge-on spiral, exhibiting a distinct disk profile. The central bulge appears prominent and has a rounded shape. There's an indication of some dust lane obscuration along the midplane of the disk. The disk shows some disturbances, possibly indicating minor interactions or recent merger activity. Star formation appears concentrated in the disk and arms, as hinted by subtle color variations along the disk, with a possible higher density in the more disturbed regions. The overall color index suggests a population of intermediate-age stars in the bulge, potentially indicating a moderate amount of recent star formation. No clear evidence of a major merger or tidal tails are observed in this image.
