The galaxy presents a flattened, elliptical morphology with a noticeable central bulge. The core exhibits a yellowish hue, suggestive of an older stellar population. Moving outwards from the core, the disk displays a blueish tint, indicating the presence of younger, hotter stars and potential ongoing star formation. The disk shows some irregularities and faint, patchy structures, possibly indicating minor disturbances or interactions. Overall, the galaxy appears to be a transition between a smooth elliptical and a more structured spiral, exhibiting characteristics of both morphological types. The disk extends a considerable distance, suggesting it may be a relatively large galaxy. There is a hint of a tidal tail or bridge on one side, suggesting a possible past interaction.
