This galaxy appears to be a spiral galaxy, exhibiting a disk-like structure. The spiral arms are moderately defined, displaying a somewhat flocculent pattern. The central bulge is of moderate size relative to the disk. There is evidence of a bar structure spanning a significant portion of the galaxy's central region. The color distribution suggests the presence of both older stellar populations within the bulge and younger, star-forming regions within the spiral arms, particularly indicated by the bluish hue in the disk. Some morphological disturbance is observed, potentially indicating past or ongoing minor interactions with another galaxy, or perhaps just internal fluctuations within the galaxy itself. The galaxy's overall shape is relatively regular, with no immediately obvious signs of a major merger in progress, though a subtle asymmetry is noted. Star formation is present, albeit at a modest rate.
