The galaxy presents as a largely smooth, elliptical or spheroidal structure. Its color profile indicates a dominant older stellar population, exhibiting a redder hue concentrated towards the central region. There's a gradual decrease in surface brightness from the core outwards, lacking any distinct spiral arm features or prominent dust lanes. The object appears well-rounded and symmetrical, suggesting a relaxed dynamical state. There's no strong indication of ongoing merger activity or tidal disturbances, but subtle irregularities cannot be ruled out due to the image's resolution.
