The galaxy presents a generally smooth, centrally concentrated morphology. The light profile exhibits a relatively high degree of radial symmetry. The core region appears yellowish-orange in color, suggesting an older stellar population. A faint, diffuse halo extends outwards from the core, exhibiting a bluer hue, implying the presence of younger, hotter stars in the outer regions. There is no obvious spiral arm structure or bar feature visible. The galaxy's shape is generally elliptical or spheroidal, leaning towards oblate. The image reveals no major signs of an ongoing merger or significant tidal disruption.
