The galaxy presents as a largely smooth, rounded structure, indicative of an elliptical or lenticular morphology. It displays a central bulge that appears bright, with a colour that skews towards yellow. There is a faint disk structure detectable, with hints of spiral arms around the bulge. These arms are not well-defined, implying either a lack of significant star formation, or that dust obscures the spiral structure. A small disturbance is visible in the galaxy, which could be a smaller galaxy being accreted by the main galaxy. Overall the colour is on the redder side, indicating the presence of older stellar populations. This galaxy is of significant mass, and is likely to be a fairly evolved system.
