This galaxy appears to be a relatively smooth, elliptical system. It presents a concentrated central bulge, exhibiting a smooth gradient of light intensity decreasing from the core. The morphology suggests a lack of significant disk structure or spiral arms. The color profile indicates a higher concentration of older stellar populations. This is particularly evident in the yellowish-orange hue of the core region. Faint blue colors can be seen in the outer regions of the halo. No obvious signs of recent major merger events are apparent. The galaxy seems to be quite isolated, with no visually apparent tidal features or close companions.
