The galaxy presents an overall elliptical morphology, exhibiting a smooth, centrally concentrated light distribution. The central region appears brighter and exhibits a yellowish-white hue, suggesting an older stellar population. Surrounding the central bulge, a fainter, more diffuse disk-like structure is observed. This outer region shows a subtle blue tint, potentially indicating the presence of younger, hotter stars and ongoing star formation, albeit at a relatively low rate. There are no prominent spiral arms or bars visible in the image. The galaxy's shape deviates slightly from perfectly circular, presenting a somewhat elongated appearance. No indications of major mergers or significant tidal disturbances are apparent, though a minor disturbance cannot be entirely ruled out.
