This galaxy presents as a single, relatively smooth object. It appears elliptical in shape, exhibiting a high degree of central concentration with a gradual decline in luminosity outward. The color profile indicates a bias toward redder wavelengths, suggesting an older stellar population. Star formation appears to be low. There are no obvious signs of spiral arm structures or dust lanes. The object is not undergoing any significant merger activity, and it does not appear to be strongly disturbed by any tidal interactions. Its morphology suggests an evolved system, with little ongoing star formation.
