The galaxy presents as a relatively smooth, centrally concentrated object, with a morphology consistent with an elliptical galaxy. Its shape is generally rounded, showing minimal deviation from a circular structure. There's a gradual decrease in luminosity from the center outwards, lacking any distinct features such as spiral arms or a prominent disk component. The color profile suggests an older stellar population, possibly with ongoing, but suppressed star formation. There is no obvious evidence of merging or tidal disturbances in the immediate vicinity. Its size appears compact, indicating a potentially high mass concentration within a relatively small physical area.
