The galaxy presents an elliptical morphology, with a smooth, centrally concentrated light distribution. The core exhibits a bright, yellowish hue, indicative of an older stellar population and potentially a supermassive black hole. Moving outward from the core, the galaxy transitions into a more diffuse and less luminous halo, characterized by a subtle gradient in color shifting towards redder tones. This suggests a decrease in the mean stellar age with increasing radial distance. The galaxy is nearly edge-on, with a slight flattening observed along its major axis, resulting in an approximate axial ratio of 0.8. There is no discernible evidence of spiral arms, dust lanes, or active star formation regions within the galaxy.
