The galaxy presents as a relatively smooth, centrally concentrated object. Its overall shape appears to be somewhat flattened, approaching a slightly elongated or elliptical morphology. A prominent central bulge is observed with high luminosity, transitioning to a more diffuse disk component at larger radii. The core exhibits a yellowish-white hue, potentially indicating an older stellar population and reduced current star formation. Hints of fainter, reddish-tinged outer regions are barely present, with some evidence of a slight tidal disturbance or possible minor interaction with a satellite galaxy, though definitive confirmation requires higher resolution data. There appears to be minimal spiral arm structure visible in the disk.
