The galaxy presents as a somewhat elongated, elliptical-like structure. The central region exhibits a concentrated, bright, yellowish-white core, possibly indicative of an older stellar population. Moving outward from the core, the light gradually diffuses, with the overall color becoming slightly redder. There appear to be no distinct spiral arm structures or prominent dust lanes visible. The galaxy appears relatively smooth, lacking significant morphological disturbances or obvious tidal features. The overall appearance is consistent with that of a moderately massive galaxy with a low star formation rate.
