The galaxy appears as a centrally concentrated object with a generally smooth morphology. There is a dominant central bulge exhibiting a high degree of roundness. Faint, diffuse features extend outwards, giving the galaxy a slight disk-like appearance. There is evidence of a low level of ongoing star formation, indicated by the presence of bluer regions throughout the galaxy, particularly within the diffuse outer areas. There may be some minor disturbance of its structure, but it is not clear if this is due to interactions with other objects.
