This galaxy exhibits a smooth, elongated morphology, suggesting it may be an elliptical galaxy viewed at an oblique angle. The central region displays a concentrated luminosity, fading gradually towards the outer edges. The color gradient transitions from a yellow-red hue in the core to a slightly bluer tint in the peripheral regions, which implies some degree of active star formation, although not dominant. There appears to be no distinct spiral arm structure or prominent dust lanes visible. The galaxy is largely undisturbed, showing no signs of ongoing or recent major merger events.
