The galaxy presents a generally smooth morphology, with a concentrated central bulge region exhibiting a yellowish-orange hue. There is some indication of a faint extension or asymmetry protruding from the main body, hinting at a possible tidal interaction or minor disturbance. The galaxy does not display well-defined spiral arms, indicating an elliptical or lenticular classification. Color gradients suggest older stellar populations dominate the central bulge, with potentially younger populations present in the peripheral regions. Overall, this appears to be a relatively massive galaxy, possibly undergoing some form of merger or accretion event.
