The galaxy presents as a smooth, elongated object. The light distribution appears relatively uniform, with a subtle concentration towards the central region. Its morphology suggests a classification as an elliptical galaxy, or potentially a lenticular galaxy viewed edge-on. The overall color is bluish, indicating the presence of a population of relatively young, hot stars contributing significantly to its luminosity, though this does not necessarily indicate a high star formation rate. There is no apparent evidence of spiral arms or a prominent disk structure. The image suggests it is a fairly isolated galaxy, with no obvious signs of recent or ongoing mergers or tidal disturbances.
