The galaxy presents a relatively smooth, elliptical morphology, appearing largely featureless in this image. Its overall shape is generally round, with a slight tendency towards elongation. The color profile indicates a concentration of light in the yellow-red part of the spectrum. The galaxy appears to have a single central core, with light intensity diminishing gradually outwards, suggesting a high degree of central concentration. There is no obvious indication of spiral arms or significant dust lanes. There are also no other merging partners clearly visible. Any disruptions are likely minor, and there is no evidence of a major merger event having recently occurred.
