This galaxy exhibits a prominent central bulge, indicative of an elliptical or lenticular morphology, though some spiral structure is present. The bulge exhibits a smooth, yellowish color, suggesting an older stellar population. The surrounding disk appears fainter and bluer, indicating the presence of younger stars and ongoing star formation. The galaxy appears moderately inclined to our line of sight. Evidence for a weak bar structure can be observed. There is also some minor disturbance in the galaxy's structure, however no major merging features are present.
