This galaxy presents as a spiral type, exhibiting a defined disk structure. Two prominent spiral arms are discernible, exhibiting a moderately wound morphology. The central bulge is large and bright, appearing as a concentrated spheroid of light. A subtle bar feature appears to be present, although not distinctly pronounced. There is no apparent evidence of significant tidal disruption or ongoing major merging events; however, some minor irregularities in the disk morphology cannot be excluded as possible disturbances. The galaxy is not seen edge-on.
