The galaxy appears as a relatively compact object with a generally smooth morphology, although subtle features suggest possible disturbances. Its core exhibits a yellowish-orange hue, indicative of an older stellar population. Fainter, bluish-white regions surround the central core, possibly indicating areas of more recent star formation. An area of increased red/orange emission is visible, indicating possible areas of dust concentration and associated star formation. There is some evidence that the galaxy is undergoing, or has undergone, some form of interaction or merger. The overall shape is not perfectly regular, showing some asymmetry. This is further suggested by the faint extensions or tidal features extending away from the main body. Based on its apparent smoothness, this galaxy might be classified as an early-type spiral or a lenticular galaxy.
