The galaxy presents a generally smooth, elongated morphology. It appears as a flattened spheroid with a distinct central bulge. The color distribution indicates a concentration of older stellar populations within the central bulge, which exhibits a yellowish hue. Moving outwards from the center, the galaxy transitions to bluer colors, suggesting the presence of younger stars and potentially ongoing star formation within the galactic disc.

There's a lack of distinct spiral arm structure, though the bluer regions hint at a disc-like morphology, and a suggestion of subtle features. There is no evidence of any major mergers or tidal disturbances in this image.
