The galaxy presents as a relatively smooth, lenticular or early-type spiral structure. The central bulge appears prominent and generally spheroidal in shape, exhibiting a yellowish-orange hue, suggesting an older stellar population. The disk component is fainter, and exhibits a slight bluish tint, suggestive of the presence of a younger stellar population undergoing active star formation. The overall color profile suggests a galaxy transitioning from active star formation to a more quiescent state, with some ongoing star formation. There is no indication of a significant major merger event, although the presence of minor disturbances or tidal features can not be ruled out based on the image. The galaxy's morphology seems regular and well-defined, showing no prominent spiral arm structures.