The galaxy presents a largely smooth morphology. The central region exhibits a bright, concentrated bulge with a yellowish hue, suggesting a population of older stars. Moving outwards, the galaxy appears to transition into a more diffuse disk. The disk structure shows hints of faint, ill-defined spiral arms, primarily discernible through subtle color variations. A slight blue tint in these regions indicates the presence of younger, hotter stars, and potentially ongoing star formation, albeit at a moderate level. The overall shape is predominantly round, with only a minor deviation towards an elongated form. There is some evidence of minor disturbances and a slight asymmetry. No obvious signs of a recent or ongoing major merger event are apparent.
