The galaxy presents as a relatively smooth, elliptical structure with a high degree of central concentration. The galaxy exhibits a slightly elongated morphology, with a subtle disk-like component potentially visible. There is a central bulge that is bright and dominates the galaxy's overall luminosity. The color profile indicates a population of older stars, contributing to its redder hue overall. There is minimal evidence of spiral arm structures or significant dust lanes within the galaxy. There may be a low level of ongoing star formation, however it is not immediately clear from the visible light spectrum. The galaxy's shape is nearly round, and the features appear to be undisturbed.
