The galaxy presents a largely smooth, elliptical morphology, showing a concentration of luminosity towards its center, suggesting a prominent galactic nucleus or core. It appears nearly circular, with no obvious disk structure or spiral arm features visible. There's a gradual decrease in luminosity from the core outwards, blending smoothly into the background sky. The light profile is relatively even, showing no significant disturbances or tidal features. The overall color profile appears to be a yellowish hue, possibly indicating an older stellar population with a relatively low ongoing star formation rate. There is no evidence of a recent or ongoing major merger event, though there may be some minor disturbances present within the galaxy.
