The galaxy presents as a roughly elliptical, unresolved object, exhibiting a smooth, centrally concentrated light distribution. There is a distinct color gradient, transitioning from a yellowish-orange hue in the core to a fainter, slightly bluer periphery. There is no visible spiral structure or prominent dust lanes, suggesting a lack of significant ongoing star formation or a more evolved stellar population. Subtle irregularities in the outer regions may hint at minor gravitational interactions. Overall, the galaxy appears to be a relatively quiescent system.
