The galaxy presents as an elliptical morphology, appearing largely smooth and featureless. The central region exhibits a strong concentration of light, with a core that is notably brighter and more yellow in color than the surrounding areas. This color suggests a potentially older stellar population dominating the nucleus. The isophotes, or lines of equal brightness, are elongated, with an apparent flattening that suggests a deviation from a perfectly spherical shape. This could indicate some rotational support. The outer regions of the galaxy show a gradual decline in brightness, fading into the background sky. A hint of blue is present in the halo, which is consistent with a younger stellar population. There is no evidence of distinct spiral arms or a well-defined disk structure. The galaxy appears relatively isolated.
