The galaxy presents an overall disk-like morphology, but without sharply defined spiral arms. The central bulge region appears bright and relatively smooth, suggesting a higher concentration of older stellar populations. This bulge appears to be spheroidal in shape. The disk component displays a mottled texture with varying luminosity, potentially indicating areas of ongoing star formation interspersed with regions of more evolved stars and dust obscuration. The galaxy does not exhibit strong signs of active galactic nucleus activity based on its smooth central region. There are no readily apparent tidal features or distorted shapes, suggesting no recent major merger events.
