The galaxy presents a largely smooth morphology, suggestive of an elliptical or lenticular type. The overall color profile indicates a bias towards redder wavelengths, potentially indicative of an older stellar population with lower ongoing star formation. The galaxy exhibits a high degree of rotational symmetry, appearing predominantly round in shape. There is no strong evidence of spiral arms, prominent dust lanes, or other distinct features often associated with actively star-forming galaxies. Faint asymmetry may be present, although image resolution makes it difficult to assess definitively.
