The galaxy appears as an elliptical or lenticular structure, exhibiting a smooth, centrally concentrated light distribution. The core region presents a yellowish hue, potentially indicative of an older stellar population. There is little evidence of spiral arm structures or significant dust lanes. The galaxy exhibits an overall morphology suggesting a relatively evolved system, possibly undergoing or having completed a phase of significant star formation in the past. Faint blue-ish regions can be seen, possibly areas of star formation or areas dominated by intermediate aged stars.
