The galaxy presents an elliptical morphology, with a concentrated central bulge exhibiting a yellowish hue, suggesting an older stellar population. There is an extended, fainter disk surrounding the bulge, indicating the possibility of a spiral structure that is not clearly resolved. The overall color gradient moves from yellow towards a slightly bluer tint away from the center, potentially implying younger stellar populations. There appears to be a degree of disturbance in the outer regions, such as lopsidedness and a faint tidal stream, which could be indicative of a minor merger or interaction with another galaxy. The galaxy lacks strong, prominent features such as distinct spiral arms or a well-defined bar, giving it a relatively smooth appearance.
