The galaxy appears as a moderately bright, centrally concentrated object. Its morphology appears relatively smooth, lacking a strong spiral arm structure or distinct bar feature. There is a slight elongation, suggesting it is not perfectly spherical, but rather more oblate in shape. There are some signs of a possible minor disturbance of gravitational influence. The overall color suggests a mature stellar population, with a relatively low rate of ongoing star formation. The galaxy likely hosts a substantial stellar mass.
