The galaxy presents a predominantly smooth, elliptical morphology. It exhibits a flattened, disk-like structure viewed at a shallow inclination angle, possibly an edge-on lenticular galaxy. The central bulge region is moderately prominent, displaying a gradual transition in luminosity and color outwards to the disk. The color gradient suggests a slightly bluer core, fading to redder hues in the outer regions of the disk. This color difference could be due to the distribution of stellar populations, with a younger, bluer population concentrated towards the center and older, redder populations dominating the outer regions. There's no prominent evidence of spiral arms or significant dust lanes. There is no pronounced evidence of any significant ongoing merger events or strong tidal disturbances, but there is a slight hint of a warp to the right edge of the disk. Based on color and morphology, the galaxy's star formation rate appears relatively low.
