The galaxy presents a slightly elongated, though generally rounded morphology. The light distribution appears relatively smooth, suggesting a lack of prominent spiral arms or distinct features such as strong dust lanes. The color profile appears mostly uniform across the galaxy's extent, hinting at a relatively homogeneous stellar population or dust distribution. There is a slight suggestion of tidal disturbances, although no clear tidal tails are visible in this image. A substantial fraction of its light is concentrated in its central region, consistent with a spheroidal galaxy shape. Based on the color indices, the galaxy is a redder color, suggesting it is a more mature galaxy. The overall appearance suggests that this galaxy may be undergoing or have recently undergone a merger event.
