The galaxy presents an elliptical morphology, appearing largely smooth and centralized. Its light profile demonstrates a concentration towards the core, exhibiting a gradual decrease in intensity outwards. The galaxy appears subtly elongated, deviating slightly from a perfectly circular shape. Color gradients are subtle, with a possible slight redder hue towards the core, perhaps indicative of an older stellar population. There is no discernable spiral structure or prominent dust lanes. No bright or particularly distinct star forming regions are clearly visible within the galaxy's structure. The galaxy appears relatively undisturbed, lacking strong tidal features or any signs of recent merger activity.
