The galaxy presents a primarily smooth morphology, exhibiting a high degree of roundness. There is a distinct central bulge, which appears to be the brightest and most concentrated region of the galaxy. The surrounding stellar distribution is relatively uniform in color and luminosity, with some subtle color variation. It presents an elliptical shape and a lack of distinct spiral arm features. The color profile appears to be dominated by older stellar populations with some regions of ongoing star formation. A significant portion of the galaxy might be the result of a galaxy merger. There are regions of minor disturbances, that do not distort the overall shape of the galaxy.