The galaxy appears to be a relatively bright object, exhibiting a smooth morphology with a subtle disk-like structure. The galaxy's core is notably brighter than its surrounding regions. There is a slight indication of disturbance, possibly a minor interaction or tidal feature, however, it is more likely a normal spiral galaxy with a slightly disturbed disk. The overall shape is more disk-like than spheroidal, leaning towards an intermediate ellipticity. Some slight asymmetry is observed, suggesting that the galaxy may not be perfectly relaxed. The dominant color is a warm hue, transitioning to redder tones in certain regions. This may be due to older stellar populations. There are a few faint blue patches visible, potentially indicating regions of active star formation within the disk.
