The galaxy presents as a centrally concentrated, elliptical-like structure. It exhibits a generally smooth morphology, with no discernible spiral arms or significant disk component visible in this observation. The central region is characterized by a bright, diffuse glow, suggesting a dense concentration of stars. Moving outward from the center, the luminosity gradually decreases, fading into a less defined halo region. The color profile appears predominantly yellow-orange, which indicates an older stellar population dominating the light output. There are some very subtle hints of disturbances, suggesting a possible minor interaction or recent accretion event, but the overall structure is largely undisturbed. The object is relatively compact in apparent size, indicating a substantial distance.
