The galaxy presents as a fairly smooth, elliptical morphology with a high degree of central concentration. The light profile appears relatively uniform across the main body, with no obvious signs of spiral arms or bar structures. There is no strong evidence of recent or ongoing major merger activity. The galaxy's color is consistent with an older stellar population, possibly indicative of relatively low star formation rates. There is a slight hint of a diffuse, extended halo surrounding the central region, although the signal is weak.
