The object is a lenticular galaxy, seen nearly edge-on. The central bulge appears prominent, exhibiting a smooth, concentrated structure. The disk component is visible as a flattened, extended structure surrounding the bulge. The disk shows a distinct redder color towards the central bulge, possibly indicating a higher concentration of older stellar populations. The outer edges of the disk are less distinct, but there appears to be a hint of bluer light, which may be caused by ongoing star formation. There is no obvious dust lane visible. The overall morphology suggests a relatively evolved system with primarily older stars, but with some indication of ongoing star formation activity in the outer regions. The galaxy is relatively isolated, showing no major signs of tidal disruption.