The galaxy presents as a single, luminous object with a generally smooth morphology. It exhibits a roughly elliptical shape with an apparent lack of defined spiral arms or a central bar. There is a color gradient observed, transitioning from a central bright blue-white core to a more diffuse, yellowish outer region. This suggests a possible transition in stellar populations, with the core potentially dominated by hotter, younger stars and the outer regions containing older, redder stars. There is also a fainter, nearby object with a similar color profile, which could be a companion galaxy, or a star cluster within the same galaxy. Given the relatively compact size and smooth appearance, this galaxy may be an elliptical galaxy or a lenticular galaxy. There is no obvious visual evidence of ongoing major mergers or significant tidal disturbances affecting the overall shape.
