The galaxy presents as a relatively compact object, characterized by a smooth, diffuse light distribution. It appears as an oblate spheroid, moderately elongated, lacking any distinct spiral arms or prominent features such as strong dust lanes or knots of star formation. Its overall color is moderately red, suggesting an older stellar population and relatively low ongoing star formation activity. There is a slightly bluer region located at the core of the galaxy. There is no evidence of a major merger, though a minor disturbance may be present, considering the slightly irregular shape. The galaxy exhibits a small angular size, implying a considerable distance. The galaxy's morphology is generally consistent with an elliptical or lenticular galaxy type.
