The galaxy appears as a slightly elongated, smooth structure, exhibiting a pale blue hue. Its morphology suggests it could be an elliptical or lenticular galaxy, with little evidence of spiral arms or prominent dust lanes. The light distribution is relatively even across the galaxy, with no particularly bright nucleus or distinct features. There are no clear signs of recent major mergers or tidal disturbances; however, a subtle asymmetry might indicate minor gravitational interactions. Overall, the galaxy presents a quiescent appearance, indicative of a relatively stable and evolved stellar population.
