The galaxy presents as an elliptical morphology, with a smooth, concentrated central bulge dominating the overall structure. The light distribution suggests a gradual decline in surface brightness moving outward from the core. The dominant color is yellowish-orange, indicating an older stellar population with relatively low levels of ongoing star formation. There is some slight bluing towards the outer regions of what could be a disk, suggesting possible presence of some younger stars. The overall shape deviates slightly from perfectly elliptical, exhibiting a small degree of elongation. There's also a slight indication of a possible minor tidal disturbance or interaction with another object, as evidenced by some asymmetry in the outer halo on one side of the galaxy.
