The galaxy appears to be an elliptical type with a smooth, centrally concentrated morphology. There is an absence of prominent spiral arms or a distinct disk-like structure. The core exhibits a bright, yellowish color, suggestive of an older stellar population. The galaxy shows a slight elongation; it is not perfectly circular, with the possibility of being an elliptical of type E3-E5 on the Hubble sequence. There may be only a slight disturbance to the galaxy from a past minor merger, with a very small chance of a larger disturbance.