The galaxy presents an elliptical morphology, appearing relatively smooth and featureless. Its shape is elongated but tending towards round. The central region exhibits a concentrated and bright core, indicative of an older stellar population, as suggested by its yellowish-white coloration. Fainter, diffuse extensions surround the core, displaying a gradient towards bluer hues at the galaxy's edges, possibly indicating regions of recent or ongoing star formation, though overall, star formation rates appear to be relatively low. The presence of some visual disturbances implies this galaxy may have experienced past interactions or minor merger events.
