The galaxy presents a smooth, elliptical morphology with a high degree of central concentration. The core exhibits a bright, yellowish-white hue, suggesting an older stellar population. The overall color profile shifts towards a redder tone in the outer regions, which may indicate a decline in ongoing star formation and an increased prevalence of older, redder stars. A faint extension is visible at the right side of the galaxy, displaying a reddish hue. This may indicate tidal disturbances but also might be an artifact. No distinct spiral arm structures or prominent dust lanes are discernible. Overall, the galaxy appears relatively undisturbed and isolated. The absence of significant blue light suggests a relatively low star formation rate.
