The galaxy exhibits a somewhat elongated, cigar-shaped morphology. There is a central, bright bulge with a yellowish hue. A fainter, disk-like structure is visible extending horizontally from the bulge. The galaxy appears to be undergoing some form of gravitational interaction or disturbance, possibly a minor merger event, as suggested by the asymmetry and a slight tidal feature. There are two regions of enhanced star formation or bluer emission, indicating the presence of younger stellar populations. The overall structure shows a degree of smoothness, suggesting a possible elliptical or lenticular classification with signs of more recent star formation. The galaxy appears to be a relatively massive system with a moderate rate of star formation.
