The galaxy presents as a moderately bright, elliptical form. Its light is largely smooth and featureless, without apparent spiral arms or distinct morphological structures. The central region appears brighter and more concentrated than the outer regions, suggesting a dense galactic nucleus. The overall color is somewhat blue, possibly indicating a component of younger stars, although the smoothness suggests older stellar populations are dominant. The shape is elongated, with a cigar-like appearance, implying a degree of rotational support. No obvious signs of ongoing merging events or major disturbances are visible, though subtle asymmetries may indicate minor interactions in its past. Overall, the galaxy seems to be a relatively undisturbed system undergoing some degree of star formation.
