The object is a spiral galaxy, presenting with prominent, well-defined spiral arms. The arms appear somewhat tightly wound towards the central bulge. The bulge itself is moderately sized relative to the disk. A bar structure seems to be present, spanning a significant portion of the galaxy's central region, showing both a strong and weak bar. There is a suggestion of multiple spiral arm counts. Visual inspection of the disk shows no distinct signs of ongoing major mergers, although the presence of minor disturbances cannot be ruled out. The color profile suggests active star formation occurring within the galaxy. The galaxy has an angular size of 2.8963 arcseconds, which when accounting for the redshift of 0.047084, translates to an estimated physical size of 2.6752 kiloparsecs.
