The galaxy presents a face-on spiral morphology. A prominent, moderately sized bulge dominates the central region, exhibiting a bright yellowish-white hue, potentially indicating an older stellar population. Distinct, well-defined spiral arms emanate from the bulge, tracing a grand design structure, with mostly two strong spiral arms. These arms display a medium winding, showing a pitch angle that is neither tightly wound nor exceptionally loose. The arms exhibit a bluer coloration compared to the bulge, indicative of younger stars and ongoing star formation. A strong bar feature is prominent throughout the galaxy, with the spiral arms emanating from the bar ends. There is no obvious major merging or tidal disruption that is occurring within this galaxy.
