The galaxy presents as a somewhat centrally concentrated object with a relatively smooth overall appearance. There is a hint of a disk structure, but it is not very prominent. The shape is generally rounded, though not perfectly so, with some elongation. There are subtle indications of minor disturbances or asymmetry in the galaxy's structure, possibly suggesting a past or ongoing interaction with another galaxy, or recent internal activity. No strong tidal features or signs of a major merger are apparent. The galaxy exhibits a color gradient, with the central region appearing brighter and potentially bluer compared to the outer regions, suggesting varying stellar populations.
