The galaxy presents as an elongated, lenticular-like structure, viewed nearly edge-on. A prominent central bulge is visible, exhibiting a smoothed, somewhat rounded morphology. The disk appears thin and is oriented approximately horizontally across the image. There is little evidence of distinct spiral arm structures or substantial dust lanes along the plane of the disk. The overall color profile suggests a mature stellar population, with a concentration of older, redder stars. The galaxy is generally smooth in appearance with no apparent signs of major disturbances.
