The galaxy presents as a relatively well-defined spiral structure. The morphology indicates a disk-dominated system with evident spiral arms. The arms display a range of winding tightness, with a dominant pattern of two spiral arms. A prominent, though not dominant, bulge is observed. There's a suggestion of a bar feature in the central region. Patches of bluer light are observed within the spiral arms, likely indicating areas of recent star formation. There may be minor disturbances present, suggestive of potential interactions. The galaxy appears to be inclined relative to our line of sight, allowing for observation of its disk structure. The overall color suggests the presence of both younger, bluer stellar populations and older, redder populations distributed throughout the galaxy.
