The galaxy appears as a concentrated, centrally-brightened object. The light profile suggests a spheroidal morphology, largely lacking distinct spiral arm structures or a prominent disk. The object exhibits a smooth appearance, with the majority of its light concentrated in a central bulge. The color indices derived from the image reveal a spectral energy distribution that is more red than blue, consistent with a galaxy dominated by an older stellar population. There may be a hint of tidal disturbance.
