This galaxy presents as a spiral type, exhibiting a distinct disk structure. The spiral arms are prominent, displaying a loosely wound morphology. Two main arms are observed emanating from the central region. A moderate-sized bulge is apparent, contributing to the overall luminosity of the galactic core. No strong bar feature is readily discernible. The galactic disk is viewed close to face-on. There are no apparent signs of major merging activity, though minor disturbances cannot be ruled out. The galaxy appears to be in a relatively isolated environment. The color gradient suggests active star formation regions within the spiral arms, although the color suggests that there is not a lot of very recent star formation. Overall, this galaxy appears to be a well-formed, classical spiral galaxy with ongoing, but not intense, star formation.
