The galaxy presents as an elliptical or lenticular-like structure, exhibiting a centrally concentrated luminosity profile that fades gradually outward. The core region displays a yellowish-white hue, suggesting a population of older, evolved stars. Fainter, bluer light surrounds the central region, potentially indicating a younger stellar population or ongoing low-level star formation. The galaxy shows a smooth overall appearance, with no strong evidence of spiral arms or significant dust lanes. There is a slight indication of tidal disturbance of a minor scale, although more extensive data would be needed to confirm this. The object is not perfectly circular, showing some degree of ellipticity, but it is closer to rounded.
