The galaxy presents an elliptical morphology with a prominent, bright central bulge, which appears nearly spherical. A diffuse, extended halo surrounds the core, gradually fading into the background sky. The galaxy is relatively smooth in texture, lacking any obvious spiral arm structures or distinct dust lanes. A slight elongation is observed along its major axis, though the overall shape remains largely circular. The color gradient indicates a population of older stars, as the core exhibits a yellower, more reddish hue, while the outer regions appear marginally bluer, likely due to a small amount of ongoing star formation. There are some signs of disturbance indicating a possible merger. Overall, the galaxy exhibits characteristics consistent with a mature elliptical galaxy, potentially undergoing or having undergone a merger event.
