This galaxy presents an elliptical morphology, appearing largely smooth and lacking distinct spiral arms. It exhibits a slight elongation. The central region appears brighter and more concentrated, indicating a possible bulge. The color profile suggests a population of older stars, with a redder hue dominating the outer regions and a slightly bluer tint toward the center, which may indicate some ongoing star formation. There is a minor disturbance in the form of asymmetry to one side of the galaxy, possibly indicating a past minor merger or interaction.
