The observed galaxy presents a relatively compact morphology. The light distribution appears concentrated toward the central region, though some fainter peripheral structure is observed. No clearly defined spiral arms or a prominent disk structure are immediately visible. It is difficult to determine an overall shape for this galaxy due to the faintness and features on the image. The galaxy has a reddish hue. The color suggests an older stellar population and/or significant dust obscuration within the galaxy. A hint of disturbance or possible ongoing minor merger cannot be fully ruled out based on the image alone. Further investigation with higher resolution data and multi-wavelength observations would be necessary to confirm such a feature.
