The galaxy presents a generally smooth and rounded morphology. Its light profile appears concentrated, with a discernible core region. The color index suggests a relatively evolved stellar population, trending towards redder wavelengths. There is no clear evidence of spiral arms or a well-defined disk structure. Minor asymmetry is present, possibly indicating a past or ongoing minor interaction, though a merger event is not immediately obvious. The overall form is consistent with an elliptical or S0 type galaxy.