The galaxy presents a generally smooth morphology. The light profile appears concentrated and elliptical. There is a high probability that this galaxy has no distinct disk-like or spiral arm features. Color gradients suggest possible variations in stellar population or dust content. Overall, the galaxy is estimated to have significant mass, as suggested by the luminosity and size, and its overall form suggests a relatively evolved system. Star formation rate is minimal. There seems to be a possibility of minor disturbance to the gravitational structure of the galaxy.