The galaxy presents as a relatively smooth, elliptical structure. It exhibits a concentrated central bulge that appears to be largely spheroidal with little visible substructure. The color is largely yellow, suggesting an older stellar population dominating its composition. There is a slight ellipticity to the overall shape, indicating it is not perfectly spherical. The galaxy lacks any visually prominent spiral arms, dust lanes, or other distinct features typically associated with younger, actively star-forming galaxies. The light is fairly diffuse, indicating it has been stretched due to cosmological redshift. It appears to be a well-formed, evolved system, likely undergoing a very low rate of star formation. No signs of a major interaction or merger are readily apparent.
