The galaxy presents a generally smooth, elliptical morphology. It exhibits a concentrated central bulge region with a relatively gradual decrease in luminosity outward. There is a notable lack of well-defined spiral arm structures or distinct dust lanes. The galaxy's overall color is a yellowish-white, suggestive of an older stellar population and a lower ongoing star formation rate. Minimal signs of tidal disturbances or interactions with neighboring galaxies are evident, indicating a relatively quiescent evolutionary state. A subtle disk structure may exist, but its presence cannot be conclusively determined given the low levels of star formation in its outer regions.
