The galaxy presents as a largely homogenous, elliptical structure with a relatively smooth appearance, showing minimal discernible features such as spiral arms or prominent dust lanes. Its color is generally consistent across its extent, with a slight concentration of luminosity towards the center, suggesting a relatively old stellar population distributed evenly throughout the galaxy. The galaxy exhibits a nearly circular morphology, deviating little from a perfectly round shape, which aligns with expectations for an elliptical galaxy viewed from a moderate distance. There is no obvious evidence of any major ongoing merging activity or significant tidal disturbances; only a slight color variance indicating the presence of minor disturbances may be occurring.
