The galaxy presents as a moderately luminous object with a discernible disk-like morphology. There appears to be some structural disturbance present within the galaxy, though not dramatically pronounced. The galaxy exhibits a somewhat asymmetric profile. Color gradients suggest ongoing star formation, indicated by the bluer hues, primarily concentrated in what appear to be spiral arm features. The central region of the galaxy appears more yellow/red, perhaps indicating an older stellar population. Overall, the galaxy appears to be a spiral galaxy, likely in an intermediate stage of its evolutionary process. The galaxy is moderately massive, with an intermediate star formation rate, and has a low specific star formation rate. 
