The galaxy presents as a moderately bright, elliptical-like structure. Its core exhibits a concentrated, yellowish hue indicative of an older stellar population. Extending outward from the core, the light gradually diminishes, transitioning into a slightly more diffuse halo. The overall morphology appears relatively smooth with no distinct spiral arm structures or prominent dust lanes visible. There is a slight asymmetry in the outer regions, possibly indicating minor gravitational interaction or disturbance but overall, it appears to be a fairly relaxed system. The color suggests a moderate redshift, with the intrinsically bluer light being shifted toward the redder end of the spectrum.
