The galaxy appears to be a relatively smooth, elliptical system. It exhibits an elongated shape, suggestive of a significant degree of flattening. The central region is brighter and appears more concentrated, gradually fading towards the outer edges. There is no readily apparent spiral structure or distinct disk features visible in the image. The galaxy's color profile appears somewhat reddish, implying an older stellar population and potentially lower levels of ongoing star formation. There may be some subtle indications of minor tidal disturbances, such as faint asymmetries in the outer halo, but overall, the galaxy seems relatively undisturbed. The majority of light seems to originate from a round central region.
