The galaxy presents as a relatively compact object with a smooth, elliptical morphology. There's a primary concentration of light with a slightly elongated form. A second, smaller concentration of light is observed nearby and appears to be connected with the main object by a subtle bridge of light. The color profile indicates varying stellar populations. The main concentration appears redder compared to the second one, which appears bluer, suggesting different ages or metallicities in these regions. The system shows signs of potential interaction or a past merger event. Tidal features are not readily apparent, however, some subtle disturbances in the isophotes could be present in higher resolution data.
