The galaxy appears as a relatively smooth, elliptical-shaped structure, with a high degree of central concentration. Its light is distributed evenly, with no apparent distinct features such as spiral arms or a bar. The color suggests an older stellar population, leaning towards redder wavelengths, indicative of a lack of significant ongoing star formation. There are indications of minor disturbances or interactions, given the slight irregularities in its overall shape, potentially caused by a past or ongoing minor merger event. The galaxy exhibits a compact morphology, with a well-defined edge.
