The galaxy presents an elliptical morphology, appearing smooth and relatively featureless at this resolution. Its color profile suggests a dominant population of older stars, with a central region exhibiting a slightly redder hue. The galaxy appears somewhat elongated, with an intermediate roundness, not perfectly spherical but also not highly elongated. There is some visual suggestion of a slight disturbance or minor interaction affecting the galaxy's structure, which may be caused by external or internal factors. The star formation rate seems to be quite low. Overall, this galaxy appears to be a massive, evolved system with a quiescent star formation history.
