The galaxy presents an elliptical morphology, appearing largely smooth with a dominant central bulge. There is a slight flattening, suggesting it is not perfectly spherical but more akin to an oblate spheroid. The color gradient shows a yellowish-white core that transitions into a faint, greenish-blue hue in the outer regions. This implies a population of older stars concentrated in the core, with some presence of younger, bluer stars in the surrounding regions. The distribution of light appears relatively uniform without any obvious signs of spiral arms or strong dust lanes. There is a possible minor disturbance of the galaxy.
