The observed galaxy presents as a spiral type, displaying a prominent, well-defined disk structure. The arms are easily discernible, exhibiting a relatively coherent pattern that is tightly wound. A strong bar feature is clearly visible bisecting the central bulge. The bulge appears moderate in size. Two spiral arms are easily discernible, with a strong spiral pattern and a medium winding tightness. No interaction or merging is apparent, although it is possible the galaxy has some minor disturbances. The core shows a bright, concentrated region, suggesting a high density of stars or possibly an active galactic nucleus, although further spectral analysis would be necessary to confirm this.
