The galaxy presents as a flattened, elliptical form, elongated along its major axis, and seen at an oblique angle. A central bulge dominates the structure with a high degree of luminosity. The light from the bulge appears yellowish-white suggesting an older stellar population. The surrounding disk appears less luminous, with a gradual fading in intensity toward the edges. There is a subtle blueish tinge. The smooth overall appearance indicates a lack of significant dust lanes. No distinct spiral arm structures are discernible. The galaxy appears relatively isolated, without signs of ongoing major mergers or strong tidal disturbances. The absence of prominent star-forming regions further suggests a galaxy past its peak star formation activity.