The galaxy presents as an approximately elliptical structure, elongated with an axis ratio that suggests a moderately flattened shape. Its color profile is dominated by a central concentration of light that is noticeably bluer than the outer regions, potentially indicating a population of younger stars. There is little sign of spiral arms or other distinct features. The surrounding halo appears relatively smooth and featureless. Some evidence suggests it is a disk galaxy viewed edge-on, but this is uncertain due to the size of the galaxy. No strong signs of mergers, major tidal disturbances, or interactions are evident, though it is difficult to assess subtle merger activity at this resolution.
