The galaxy presents as a centrally concentrated, elliptical-like structure with a generally smooth appearance. It is largely featureless, showing no prominent spiral arms or distinct bars. The light profile appears to be relatively uniform, decreasing gradually from the core outward. The color appears to be primarily yellowish-orange, possibly indicating an older stellar population with lower levels of ongoing star formation. There may be some very subtle hints of greenish-blue on the edges of the galaxy, possibly indicating that this is where any star formation may be concentrated. There is no significant dust lane obscuring the view of the core. It appears as a single, isolated galaxy, showing no signs of ongoing major merger events or substantial tidal disturbances from close neighbors. The galaxy is fairly compact, with no pronounced extended halo or large-scale structures.
