The galaxy appears as a relatively smooth, elliptical structure. It exhibits a generally rounded morphology, with no immediately obvious disk or spiral arm features. The galaxy’s core is a bright, concentrated region. A smooth decrease in luminosity is observed moving outwards from the center, indicating a lack of prominent substructure. The color profile suggests a population of older stars. There are no obvious signs of ongoing major mergers, although subtle disturbances cannot be completely ruled out given the image resolution. Overall, the galaxy presents as a mature system likely with an absence of current intense star formation.
