The galaxy presents a flattened, elliptical morphology, viewed at a significant inclination. The central region exhibits a high concentration of light, appearing yellowish-orange suggesting an older stellar population. Moving outwards from the core, the color gradually shifts towards a bluer hue in the outer regions of the disk. This implies more recent star formation occurring in the periphery. The disk appears relatively smooth with no prominent spiral arm structure visible, indicating that the galaxy is not undergoing significant merger activity. Faint hints of dust lanes may be present, but the image resolution is not high enough for definitive identification. The overall structure and color gradients suggest a galaxy with a mix of stellar populations and a relatively quiescent star formation history.
