The galaxy presents as a relatively small, elongated structure. Its morphology suggests it is an elliptical galaxy, characterized by a smooth, diffuse light distribution. There is no clear evidence of spiral arms or a prominent galactic disk. The color appears to be primarily red, indicating an older stellar population dominated by red giant stars. This further supports the classification as an elliptical galaxy, as these systems tend to have less active star formation.

There might be a slight distortion in its shape, suggesting a possible past interaction or merger with another galaxy, although it appears to be primarily relaxed now. The overall color profile and lack of distinct features indicate that the galaxy has likely exhausted most of its gas and dust reserves for star formation and is therefore experiencing a low rate of star formation.
