The galaxy presents as a somewhat elongated, smooth structure, with a concentrated central bulge that appears diffuse and unresolved at this resolution. The color profile appears to have a bias towards redder wavelengths, possibly indicating an older stellar population and a reduced rate of star formation. The morphology suggests a system that may be in the process of merging or experiencing some form of gravitational disturbance, evident by the slight asymmetry. There is no clear disk structure. Its overall appearance suggests it is an evolved galaxy with a substantial mass, and lies at a considerable distance.
