The galaxy presents a largely smooth morphology, appearing somewhat elliptical in shape, although some slight irregularities are visible within the overall structure. There is a concentration of light toward the center, giving it a brighter, more luminous core. The color is primarily a yellow-orange hue, suggesting an older stellar population with relatively low recent star formation activity. Subtle variations in color and brightness suggest some internal structure, but there are no prominent spiral arms or other disk-like features immediately apparent. There is no significant morphological distortion visible. Overall, the galaxy appears to be a relatively isolated and undisturbed system.
