The galaxy presents as a single, relatively smooth object. There appears to be a central, concentrated bulge region with a yellowish hue, suggestive of an older stellar population. A faint, more diffuse disk surrounds the bulge, exhibiting a slight greenish tint. This could indicate some ongoing star formation, though not at a particularly vigorous rate. The overall shape of the galaxy is somewhere between round and elliptical, lacking a highly defined spiral structure or bar. The outer edges of the galaxy are not well-defined. Evidence suggests the galaxy may be undergoing some form of interaction or disturbance, with possible minor irregularities. The classification of its morphology leans towards a smooth structure.
