The galaxy presents as a spiral with tightly wound arms. The central bulge is prominent and appears moderately sized relative to the overall disk. The galaxy disk shows a complex structure with some patchy regions of star formation along the spiral arms. There are no obvious signs of a strong bar feature bisecting the bulge. The overall color suggests a mixture of stellar populations, with a yellowish central region indicating older stars, and bluer regions in the disk, potentially indicating ongoing or recent star formation. There is no obvious strong tidal features that would indicate a recent major merger. The spiral arms show no strong irregularities or disturbances.
