The galaxy appears as an elliptical-like structure with a concentrated, bright central bulge. A faint disk is visible around the bulge, though it is difficult to resolve any spiral arm structures. The galaxy exhibits a smooth overall appearance, though there is some indication of minor disturbances in its morphology. Color gradients show a yellow/white core, with a bluer hue at the edges of the disk. This color profile suggests a population of older stars at the core, and a younger stellar population on the outer edges. There is no obvious evidence of major ongoing merging activity. Overall the galaxy seems to be in a relatively stable state. 
