The galaxy presents a roughly elliptical morphology, though it is somewhat irregular in appearance, hinting at a potential ongoing interaction. It is dominated by a bright central region. A disk-like structure may be present, but is not clearly defined. The color gradient suggests a complex stellar population distribution, with bluer hues concentrated in the central region, which may indicate younger star formation. There are some minor disturbances and color irregularities that suggest possible interactions with another galaxy. Fainter and more diffuse outer regions extend from the main body. The galaxy's overall structure suggests it may be undergoing or have recently undergone a merger event.
