The galaxy appears as a centrally concentrated object, exhibiting a generally smooth morphology. A slight ellipticity is observed, but the shape is close to round. The central region is brighter, potentially indicating a nucleus or bulge. Fainter, diffuse light extends outwards from the core, with a subtle hint of a disc-like structure. No strong spiral arms or distinct features are readily apparent. Based on the galaxy's color, it appears to be a fairly mature system, but there may be low levels of ongoing star formation occurring. There is a subtle disturbance in the morphology that suggests there is some gravitational interaction. The galaxy could have undergone a minor merger in the past.