The galaxy presents as a generally smooth, centrally concentrated object, likely an elliptical or lenticular type. The core region exhibits a bright, yellowish hue, indicating an older stellar population and a lack of significant ongoing star formation. A subtle, greenish tint surrounds the core and extends outwards, possibly indicating some low-level star formation or ionized gas. The galaxy's overall shape appears somewhat round, with no obvious signs of a disk component or spiral arms. There are no obvious tidal tails or morphological disturbances present that would indicate a recent or ongoing merger event; however, there is a hint of irregularity to its edge. The galaxy shows significant signs of being a relatively massive object.
