The galaxy presents a generally smooth, elliptical morphology. The central region exhibits a high concentration of light, appearing bright yellow-white, indicative of an older stellar population. The light intensity gradually decreases with radial distance from the center. A faint, extended halo surrounds the core, with colors transitioning towards redder hues, suggesting a decline in younger, bluer stars in the outer regions. There's no readily apparent spiral arm structure or dust lane obscuration visible. The galaxy appears relatively undisturbed, showing no major signs of recent merger activity or tidal interactions with other galaxies. The overall shape approximates roundness, with only a slight deviation from a perfect circle.
