The galaxy presents as an elliptical-type system. It appears largely smooth in texture, with a concentrated central bulge. The color profile suggests an older stellar population, dominated by redder wavelengths and implying a cessation or significant reduction in star formation. The morphology exhibits high degree of roundness, with only slight deviation from a perfectly circular form. There is no clear visual evidence of ongoing mergers or tidal disturbances, although some subtle asymmetry cannot be ruled out at this resolution.
