The galaxy presents as an elongated, elliptical form. Its central region exhibits a smooth, concentrated light distribution. A subtle color gradient is observed, with the core appearing somewhat bluer compared to the outer regions. The galaxy's disk is observed to be very thin and is oriented nearly edge-on from our viewing perspective. There is an absence of prominent spiral arm structures or significant dust lane features, suggesting a relatively quiescent state. It appears to be of intermediate size, consistent with a mass of roughly 1 billion solar masses. The overall structure suggests a relatively evolved system with a moderate rate of star formation.
