The galaxy presents as a spiral type, exhibiting a prominent disk structure with well-defined spiral arms. These arms appear loosely wound, extending outward from the central region. A subtle central bulge is observable, though not overwhelmingly dominant in size relative to the disk. There is no strong evidence of a prominent bar structure within the galactic core, though a subtle asymmetry suggests a possible weak bar.

The galaxy shows signs of ongoing star formation, particularly within the spiral arms, indicated by a bluer color and a mottled texture. No major tidal disturbances are readily apparent, but there is some degree of asymmetry, potentially suggestive of a minor interaction. Overall, the galaxy appears to be relatively isolated and not undergoing any major merging activity.
