The galaxy presents a generally smooth morphology, with an overall elliptical shape. The central region appears as a bright, concentrated bulge, exhibiting a yellowish-white hue, suggestive of an older stellar population. Moving outward from the core, the galaxy displays a more diffuse, bluish disc. This bluer color in the outer regions indicates the presence of younger, hotter stars, implying ongoing star formation. The galaxy shows moderate elongation. There is no obvious evidence of a major ongoing merger, though some minor disturbances may be present within the disc.
