The galaxy appears to be a relatively bright, yellowish-white object. The central region exhibits a high degree of luminosity, suggesting a concentrated stellar population or active galactic nucleus. Moving outwards from the core, the luminosity gradually decreases, forming a somewhat diffuse halo. The overall shape is elongated and somewhat irregular, neither perfectly spherical nor a clearly defined spiral. There is a hint of some features or disturbances within the galaxy's morphology, suggesting possible interactions or internal activity, but no obvious spiral arms. The smooth appearance with some faint features suggests a transition between a pure elliptical and early spiral type morphology.
