The galaxy presents as a spiral galaxy with a prominent, moderately sized bulge. Two spiral arms can be distinctly visualized, tightly wound around the galactic nucleus. The galaxy exhibits a well-defined disk structure. A strong bar feature traverses through the central bulge region. The morphology suggests that this galaxy is not undergoing any significant merger activity, with a minimal disturbance in its overall structure. The observed color gradients suggest a mix of stellar populations, likely with older stars dominating the bulge, while younger, bluer stars reside in the spiral arms. The spiral arms have some moderate star forming regions as indicated by their blue tint.
