The galaxy presents an overall smooth, elliptical morphology. The central region exhibits a concentrated, bright, and slightly reddish hue, possibly indicating an older stellar population. Moving outwards from the core, the color shifts towards a less intense yellowish-white, suggesting a mixture of stellar ages. There appears to be a minor disturbance within the galaxy, evidenced by the uneven distribution of light in one area, though not definitively a major merger event. The isophotes suggest a slight deviation from perfect ellipticity.
