The galaxy presents an elliptical morphology, with a noticeable central bulge exhibiting a yellowish hue, indicative of an older stellar population. The disk component, while present, appears less prominent and displays a bluer color, suggesting ongoing star formation. There's a slight asymmetry observed in the outer regions of the disk, potentially indicating a past or ongoing minor merger event or tidal disturbance. Overall, the galaxy appears to be a transitioning system, displaying characteristics of both elliptical and spiral galaxies, with evidence of past interactions influencing its morphology.
