The galaxy appears as a centrally concentrated object with a smooth, diffuse morphology. It exhibits a generally elliptical shape, tending towards roundness, with a slight elongation that is not cigar-shaped. There's no visible evidence of spiral arms or a distinct disk structure. The light distribution appears relatively uniform, with a central region that is brighter and more intensely colored, likely indicating a higher density of stars or a more active galactic nucleus. There is no obvious major disturbance to the overall structure, suggesting no recent or ongoing major merger events. Faint color variations are present, with the inner regions trending towards redder hues, potentially indicating an older stellar population or the presence of dust obscuration. There is no sign of clumpy star-forming regions or prominent blue colors that would signify ongoing, widespread star formation.
