The galaxy presents as a centrally concentrated object with a smooth overall appearance. The core exhibits a reddish hue, suggestive of an older stellar population. Proceeding outward from the core, a diffuse, bluish halo is observed. There is a subtle indication of spiral arm structures, but the features are not well-defined. There is no sign of any merging activity. The overall morphology indicates a relatively evolved system with a notable population of older stars at its core and ongoing, though potentially low, levels of star formation in its outer regions. The shape is somewhere between a disk and a sphere.
