The galaxy presents as a centrally concentrated, relatively smooth structure. The morphology appears primarily elliptical or spheroidal, with little evidence of spiral arms or a distinct disk component. The central region exhibits a brighter, more luminous concentration of light, suggesting a bulge or nucleus. The color profile indicates a redder hue, especially in the core, which might be indicative of an older stellar population. The outer regions are less defined and appear to fade gradually into the background sky. There is no obvious indication of a major ongoing merger, although there may be a very slight asymmetry in the outer halo.
