The galaxy appears to be a somewhat elongated structure, possibly a spiral or lenticular galaxy viewed at an angle. The light distribution seems relatively smooth, with a concentrated central bulge, which emits a yellowish-white light, suggesting an older stellar population. Fainter blue regions are observed, which may indicate regions of more recent star formation, although the exact morphology is difficult to discern. There is a suggestion of a slight disturbance in the galaxy’s form which may be the result of a minor gravitational interaction.
