The galaxy exhibits an elliptical morphology, appearing elongated with a smooth and centrally concentrated light distribution. Its color profile indicates a dominant population of older stars, with a reddish-yellow hue concentrated towards the core. There's no discernable presence of spiral arms or dust lanes. The galaxy appears relatively undisturbed, showing no significant signs of recent mergers or tidal interactions. The isophotes suggest a high degree of flattening, indicating a possible oblate spheroidal shape.
