Observed at Right Ascension 207.080530 and Declination 65.212942, the galaxy presents as a relatively small, elongated object. The overall morphology appears to be disk-like, with a significant amount of internal structure visible. There is some evidence of features and a potential spiral arm structure.

The galaxy's color gradient shows a subtle trend, with the central regions appearing slightly redder compared to the outer edges. This could indicate differing stellar populations or dust distributions. The overall light distribution is somewhat uneven, suggesting possible active star-forming regions within the disk. There may be minor distortions in the galaxy's structure, hinting at past or ongoing interactions, but the object generally appears undisturbed. 
