The galaxy presents as a spiral galaxy with a well-defined, bright central bulge. The bulge exhibits a yellowish hue, suggestive of an older stellar population. Spiral arms emanate from the central bulge, displaying a bluish tint, likely indicative of ongoing star formation. The arms are relatively tightly wound and are symmetrical around the galaxy's center. The galaxy's overall shape is elliptical with high axial symmetry. There is no visual evidence of a bar structure in the center of the galaxy. There is no strong evidence of merging or major tidal disturbances.
