The galaxy appears as a centrally concentrated, smooth, and rounded object. Its color profile suggests a relatively older stellar population, with a dominant yellowish hue. There is no distinct spiral arm structure or bar feature visible; instead, the light is distributed in a diffuse manner. The shape appears mostly spherical. There is no obvious sign of a major ongoing merger, although subtle morphological irregularities might indicate minor disturbances or past interactions. The galaxy's overall appearance is consistent with an elliptical galaxy, with its high level of smoothness and high degree of roundness. There is also some evidence to suggest that this galaxy is relatively massive, based on the amount of light it emits.
