The galaxy presents as a somewhat elongated, lenticular structure, likely seen edge-on or at a high inclination. The central bulge appears prominent and displays a yellowish-orange hue, indicating an older stellar population. The disk component exhibits a bluer color, suggestive of ongoing or recent star formation, though this is not extensive. The galaxy's morphology appears relatively undisturbed, showing no strong signs of tidal interactions or recent merger events. There is a suggestion of faint spiral arm structures extending from the bulge, but they are not well-defined. The light distribution is concentrated towards the center, with a gradual decrease in brightness towards the outer regions of the disk. Overall, the galaxy seems to be an intermediate-mass system that is evolving and quiescent.
