The galaxy presents an elliptical morphology, appearing relatively smooth and centrally concentrated. Its shape is somewhat elongated but not strongly so, leaning towards a more oblate spheroidal form. The galaxy exhibits a color gradient, with the central region appearing more yellow, suggesting an older stellar population and/or dust obscuration. There is a marginal presence of a disk structure. Overall, there is no strong visual evidence of significant ongoing star formation within the galaxy's main body. There is no indication of major disturbances or merging events in the galaxy's recent history.